Gaia Science Alerts Working Group wiki_gsawg https://gsawg.wiki.ast.cam.ac.uk/index.php?title=Main_Page MediaWiki 1.35.14 first-letter Media Special Talk User User talk Gaia Science Alerts Working Group Gaia Science Alerts Working Group talk File File talk MediaWiki MediaWiki talk Template Template talk Help Help talk Category Category talk 0 1 1 2009-07-02T14:12:29Z MediaWiki default 0 wikitext text/x-wiki <big>'''MediaWiki has been successfully installed.'''</big> Consult the [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for information on using the wiki software. == Getting started == * [http://www.mediawiki.org/wiki/Manual:Configuration_settings Configuration settings list] * [http://www.mediawiki.org/wiki/Manual:FAQ MediaWiki FAQ] * [https://lists.wikimedia.org/mailman/listinfo/mediawiki-announce MediaWiki release mailing list] bd962048d95fbb6b6b514885867811db20a5476b 5 1 2009-07-02T17:06:01Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''MediaWiki has been successfully installed.'''</big> 312f6387ab4d5a527da11716f99b3bcd5e41fcfb 8 5 2009-07-02T17:10:41Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Welcome to the web site of the Gaia Science Alerts Working Group!'''</big> The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. '''Every one interested in the subject is invited to contribute to this website!''' ---- ''This page is maintained by [[Lukasz Wyrzykowski | user:lukasz]]. Contact me for the password. '' ---- 90d75501d7d17cfa05ba865216ddf5009d024890 10 8 2009-07-02T17:13:18Z Lukasz 2 wikitext text/x-wiki <big>'''Welcome to the web site of the Gaia Science Alerts Working Group!'''</big> The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. '''Every one interested in the subject is invited to contribute to this website!''' ---- ''This page is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. Contact me for the password. '' ---- 5f5148ed6b44981e5ad6bfd0dba19a00c78573b2 37 10 2009-07-07T14:20:08Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. '''Every one interested in the subject is invited to contribute to this website!''' ---- ''This page is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. Contact me for the password. '' ---- 63a2e1ad1f41ecdbd2f3898d7c00dbc658b16b62 6 2 2 2009-07-02T16:25:05Z Gsawgwikiadmin 1 Cambridge radiotelescopes logo - wide. wikitext text/x-wiki Cambridge radiotelescopes logo - wide. 6dea2fc0063ba7f8d1eb3833ce6c35a64d0d69e3 8 3 3 2009-07-02T17:02:32Z Gsawgwikiadmin 1 Created page with '* navigation ** mainpage|mainpage-description ** links|links ** People|people * Science ** Triggers ** Contaminants * Alerts ** detection-system|detection-system ---- ** cu...' wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|links ** People|people * Science ** Triggers ** Contaminants * Alerts ** detection-system|detection-system ---- ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX c8ae4c3978478951e4f70ff767bd59bada76c362 4 3 2009-07-02T17:04:30Z Gsawgwikiadmin 1 wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection-system|Detection System ** verification-phase|Verification phase ** follow-up|Follow-up * SEARCH * TOOLBOX 45dd5b725dcd42f1577199b841e905ccb9a40039 19 4 2009-07-02T17:43:02Z Gsawgwikiadmin 1 wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up * SEARCH * TOOLBOX 760ad67396e52fd0268024870499fac512a68cf3 12 4 6 2009-07-02T17:06:11Z Gsawgwikiadmin 1 Created page with 'Consult the [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for information on using the wiki software. == Getting started == * [http://www.mediawiki.org/wiki/Manual...' wikitext text/x-wiki Consult the [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for information on using the wiki software. == Getting started == * [http://www.mediawiki.org/wiki/Manual:Configuration_settings Configuration settings list] * [http://www.mediawiki.org/wiki/Manual:FAQ MediaWiki FAQ] * [https://lists.wikimedia.org/mailman/listinfo/mediawiki-announce MediaWiki release mailing list] 4f1d112df885795f61f8be34232a8d8b3d9fc5a0 7 6 2009-07-02T17:07:42Z Gsawgwikiadmin 1 wikitext text/x-wiki Consult the [http://meta.wikimedia.org/wiki/Help:Contents User's Guide] for information on using the wiki software. == Getting started == * [http://www.mediawiki.org/wiki/Manual:Configuration_settings Configuration settings list] * [http://www.mediawiki.org/wiki/Manual:FAQ MediaWiki FAQ] * [https://lists.wikimedia.org/mailman/listinfo/mediawiki-announce MediaWiki release mailing list] == Basic text formatting == You can format the page using Wikitext special characters. {|width="80%" border="1" cellpadding="2" cellspacing="0" |- !What it looks like !What you type |- | You can ''italicize text'' by putting 2 apostrophes on '''each''' side. 3 apostrophes will '''embolden the text'''. 5 apostrophes will '''embolden''' and ''italicize'' '''''the text'''''. (Using 4 apostrophes doesn't do anything special -- <br>the last pair are just '''' left over ones'''' that are included as part of the text.) |<pre> You can ''italicize text'' by putting 2 apostrophes on each side. 3 apostrophes will '''embolden the text'''. 5 apostrophes will '''embolden''' and ''italicize'' '''''the text'''''. (Using 4 apostrophes doesn't do anything special -- <br /> the last pair are just ''''left over ones'''' that are included as part of the text.) </pre> |- | A single newline generally has no effect on the layout. These can be used to separate sentences within a paragraph. Some editors find that this aids editing and improves the ''diff'' function (used internally to compare different versions of a page). But an empty line starts a new paragraph. When used in a list, a newline ''does'' affect the layout ([[#lists|see below]]). |<pre> A single newline generally has no effect on the layout. These can be used to separate sentences within a paragraph. 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Please do not start a link or ''italics'' or '''bold''' text on one line and end on the next. </pre> |- |You should "sign" your comments on talk pages: <br/> - Three tildes gives your signature: [[User:Example|Example]] <br/> - Four tildes give your signature plus date/time: [[User:Example|Example]] 07:46, 27 November 2005 (UTC) <br/> - Five tildes gives the date/time alone: 07:46, 27 November 2005 (UTC) <br/> |<pre> You should "sign" your comments on talk pages: - Three tildes gives your signature: ~~~ - Four tildes give your signature plus date/time: ~~~~ - Five tildes gives the date/time alone: ~~~~~ </pre> |} 6f92a152698c9139b909118c4f032b612ae3c79e 2 5 9 2009-07-02T17:12:45Z Lukasz 2 Created page with ''''Lukasz Wyrzykowski''' Institute of Astronomy University of Cambridge Madingley Road CB3 0HA Cambridge UK email: wyrzykow_ast.cam.ac.uk tel. (44) 1223 337504 www: [[ht...' wikitext text/x-wiki '''Lukasz Wyrzykowski''' Institute of Astronomy University of Cambridge Madingley Road CB3 0HA Cambridge UK email: wyrzykow_ast.cam.ac.uk tel. (44) 1223 337504 www: [[http://www.ast.cam.ac.uk/~wyrzykow http://www.ast.cam.ac.uk/~wyrzykow]] bb33550b796d5389e1451946e1fd0368f1fd18d2 0 6 11 2009-07-02T17:27:19Z Lukasz 2 Created page with '== Various links related to Gaia and Science Alerts == * [[http://www.rssd.esa.int/index.php?project=Gaia|Gaia]] Main Gaia page in ESA * [[http://obswww.unige.ch/~eyer/VSWG/|Va...' wikitext text/x-wiki == Various links related to Gaia and Science Alerts == * [[http://www.rssd.esa.int/index.php?project=Gaia|Gaia]] Main Gaia page in ESA * [[http://obswww.unige.ch/~eyer/VSWG/|Variable Stars Working Group]] This is a closely related working group. The objectives include: the estimation of the total number of variable objects detected by Gaia, the algorithm for variable object detection, the algorithm for variable object classification. * [[http://www.mpia-hd.mpg.de/GAIA/|Classification Working Group]] The goal of this working group is to develop the necessary methods to classify all of the objects observed and to determine meaningful astrophysical parameters (such as stellar effective temperatures, compositions, radii and so forth). This will make use not only of the multiband photometry, but also the parallaxes, the proper motions (e.g. for QSO detection), the radial velocity spectrum (yielding much additional information on bright targets) and variability data. * [[http://www.ast.cam.ac.uk/~vasily/ogle_som/index.html|Light curve classification with SOMs]] Page of Vasily Belokurov on application of Self-Organizing Maps (Kohonen maps) for light curve classification on the OGLE variable stars. a17fe2e83acb1cedfc06bbe9997605b13bac57e7 12 11 2009-07-02T17:33:36Z Lukasz 2 wikitext text/x-wiki == Various links related to Gaia and Science Alerts == * [http://www.rssd.esa.int/index.php?project=Gaia Gaia] Main Gaia page in ESA * [http://obswww.unige.ch/~eyer/VSWG/ Variable Stars Working Group] This is a closely related working group. The objectives include: the estimation of the total number of variable objects detected by Gaia, the algorithm for variable object detection, the algorithm for variable object classification. * [http://www.mpia-hd.mpg.de/GAIA/ Classification Working Group] The goal of this working group is to develop the necessary methods to classify all of the objects observed and to determine meaningful astrophysical parameters (such as stellar effective temperatures, compositions, radii and so forth). This will make use not only of the multiband photometry, but also the parallaxes, the proper motions (e.g. for QSO detection), the radial velocity spectrum (yielding much additional information on bright targets) and variability data. * [http://www.ast.cam.ac.uk/~vasily/ogle_som/index.html Light curve classification with SOMs] Page of Vasily Belokurov on application of Self-Organizing Maps (Kohonen maps) for light curve classification on the OGLE variable stars. 917b564de15f3dbaec1ebcc57f200e95639d2675 0 7 13 2009-07-02T17:36:09Z Lukasz 2 Created page with '==People contributing to the Science Alerts Working Group== ''Add your name here if you contribute.'' * Institute of Astronomy, Cambridge, UK ** [[user:Lukasz|Lukasz Wyrzykowski...' wikitext text/x-wiki ==People contributing to the Science Alerts Working Group== ''Add your name here if you contribute.'' * Institute of Astronomy, Cambridge, UK ** [[user:Lukasz|Lukasz Wyrzykowski]] ** [[user:STH | Simon Hodgkin]] ** [[user:Vasily | Vasily Belokurov]] 00054269cfdaf65310a8d82ac74522afc888418c 0 8 14 2009-07-02T17:38:07Z Lukasz 2 Created page with '''' Please expand this section with your favourite types of possible alerts or contaminants. The most useful information would be the number statistics, amplitude and timescale, ...' wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts or contaminants. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] 72c3eacb75661e2eeba415ff00ce51d2e3c3f435 16 14 2009-07-02T17:40:15Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] f8eebad36d08f6c17804740cd6f131eed29f16b8 28 16 2009-07-03T13:41:57Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:Other | Other rare transients]] 90907b63d4c2859bead18e3d4328b3ecb3ba909e 38 28 2009-07-10T12:13:17Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] 405ceb65a5d93f507738b654fcb649d76f6afb5a 47 38 2009-07-10T13:43:31Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This tables is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} pc^{-3} yr^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} yr^{-1}L_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} yr^{-1}L_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} yr^{-1}L_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} yr^{-1}</math> | |} a96453cd9d494af192e0ebabb550cb5389d55836 48 47 2009-07-10T14:35:28Z Lukasz 2 /* Table of transients */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} c3201ab1b59a979b38701a28c4b9f6c820efaa34 49 48 2009-07-10T15:06:46Z Lukasz 2 /* Table of transients */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:DNe | Dwarf/classical novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} d3519991c1eeb7b220707f42b29d146e4acec28a 50 49 2009-07-10T16:39:31Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} 7dba2d945632301eb1dc4328c72a25654891eff1 0 9 15 2009-07-02T17:39:54Z Lukasz 2 Created page with '''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplit...' wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:Be | Be-type stars]] d67f221655daf99f431c08367d3c4ff2a8965526 0 10 17 2009-07-02T17:41:22Z Lukasz 2 Created page with '* '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the ...' wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) 5f7e9852033f0b410c5e506eca71252dc05d019c 20 17 2009-07-02T17:43:26Z Gsawgwikiadmin 1 moved [[Detection-system]] to [[Detection system]] wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) 5f7e9852033f0b410c5e506eca71252dc05d019c 24 20 2009-07-03T13:19:40Z Lukasz 2 wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC_branches%2FCU5%2Fdocs%2Fpersonal%2Flwyrzyko%2Fdocs%2FFluxAlertsManual%2Ffluxalertsmanual.pdf Gaia WebSVN] (Gaia password required), or [[fluxalertmanual.pdf|here]]. acc552d767dd0a233537bf56c2745bf0174910b9 26 24 2009-07-03T13:25:31Z Lukasz 2 wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC_branches%2FCU5%2Fdocs%2Fpersonal%2Flwyrzyko%2Fdocs%2FFluxAlertsManual%2Ffluxalertsmanual.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. 48ceb3319ad533e19cea5a04b449382ab687f52e 27 26 2009-07-03T13:25:43Z Lukasz 2 wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC_branches%2FCU5%2Fdocs%2Fpersonal%2Flwyrzyko%2Fdocs%2FFluxAlertsManual%2Ffluxalertsmanual.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. 6ca057ad185c69ccff182b19277dc536dca49c79 0 11 18 2009-07-02T17:41:45Z Lukasz 2 Created page with 'Main aim of the Verification Phase is to verify the robustness of the issued alerts and confirm them with the dedicated set of follow-up telescopes. This should reveal all necess...' wikitext text/x-wiki Main aim of the Verification Phase is to verify the robustness of the issued alerts and confirm them with the dedicated set of follow-up telescopes. This should reveal all necessary adjustments to be done in the detection algorithm to assure the best and the most robust performance later on. Verification Phase will last for 2-3 months and is planned to take place as early in the mission as possible, as soon as the alerting system is ready to perform. Currently, it seems it will happen only after the first cycle (half a year, i.e. late 2012/early 2013), as the accumulated data ("baseline flux") will not be available before. fa465afaea1b50e4be83d5b723c3664cab71bca0 22 18 2009-07-02T17:43:47Z Gsawgwikiadmin 1 moved [[Verification-phase]] to [[Verification phase]] wikitext text/x-wiki Main aim of the Verification Phase is to verify the robustness of the issued alerts and confirm them with the dedicated set of follow-up telescopes. This should reveal all necessary adjustments to be done in the detection algorithm to assure the best and the most robust performance later on. Verification Phase will last for 2-3 months and is planned to take place as early in the mission as possible, as soon as the alerting system is ready to perform. Currently, it seems it will happen only after the first cycle (half a year, i.e. late 2012/early 2013), as the accumulated data ("baseline flux") will not be available before. fa465afaea1b50e4be83d5b723c3664cab71bca0 0 12 21 2009-07-02T17:43:26Z Gsawgwikiadmin 1 moved [[Detection-system]] to [[Detection system]] wikitext text/x-wiki #REDIRECT [[Detection system]] c87fe82e25a347d084cca80eef139775718f0140 0 13 23 2009-07-02T17:43:47Z Gsawgwikiadmin 1 moved [[Verification-phase]] to [[Verification phase]] wikitext text/x-wiki #REDIRECT [[Verification phase]] efe27f8a4201cbcab88cc246cda0b223fc16f08f 6 14 25 2009-07-03T13:20:14Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 15 29 2009-07-03T14:05:48Z Lukasz 2 Created page with '== NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac...' wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) [[Media:NGC300-OT-lightcurve.png]] bcb38542985e153b2b37fca4e313610721c6269b 30 29 2009-07-03T14:06:10Z Lukasz 2 /* NGC300-OT */ wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) [[File:NGC300-OT-lightcurve.png]] 81deb358f7e496206c955cd42659efdd1ec2814c 32 30 2009-07-03T14:11:31Z Lukasz 2 /* NGC300-OT */ wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of masive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star [[File:NGC300-OT-lightcurve.png]] ---- 5bbb9a8a76a5ddf7db23268ba589eeaaee49ee7d 6 16 31 2009-07-03T14:06:36Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 17 33 2009-07-07T13:00:16Z Lukasz 2 Created page with '== Various instruments suitable for Gaia alerts response == * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in M...' wikitext text/x-wiki == Various instruments suitable for Gaia alerts response == * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 6750a51bea17a964074d6880aec674f3cb360795 34 33 2009-07-07T13:00:35Z Lukasz 2 /* Various instruments suitable for Gaia alerts response */ wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * e4768ad1e9d4f5b58da70b0d0614d3833da3691a 35 34 2009-07-07T13:06:32Z Lukasz 2 /* Current and future instruments suitable for Gaia alerts response */ wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * MAGIC Telescopes ([http://arxiv.org/abs/0907.1001 Garczarczyk et al. 2009], [http://arxiv.org/abs/0907.0843 Anderhub et al. 2009], [http://axiv.org/abs/0907.1046 Berger et al. 2009]) * a65c66e67b85ae8ffb3c7e7209023654ddf9e097 36 35 2009-07-07T14:02:56Z Lukasz 2 /* Current and future instruments suitable for Gaia alerts response */ wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * e4768ad1e9d4f5b58da70b0d0614d3833da3691a 0 18 39 2009-07-10T12:22:49Z Lukasz 2 Created page with 'FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri]] Plot from [http://www.ta3...' wikitext text/x-wiki FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. cf4b9e3de55cd2eca3e70a0482ff9b2f282bd3dd 41 39 2009-07-10T12:36:30Z Lukasz 2 wikitext text/x-wiki FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present More general characteristics of FUors, based on other examples * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) * Spectra: F or G supergiants * Some of them are embedded in nebulas * OO Serpentis is newly discovered another example of FU Ori [http://arxiv.org/abs/0705.1231 Kospal et al. 2007]. 9715ccbd37051e0957f3d5ee2e6a8a536e08a22a 42 41 2009-07-10T12:44:05Z Lukasz 2 wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === === OO Serpentis === OO Ser ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]) is an object discovered with ''Infrared Space Observatory'', similar to FUors and EXors. 5d43d5dc98c5bbec08352b4588d17e127ab0bd9c 43 42 2009-07-10T13:00:27Z Lukasz 2 /* OO Serpentis */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === === OO Serpentis === OO Ser was discovered in 1995 and is similar to FUors and EXors. It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). f403239cc9d2754dfa9f45e4814755b5405e5d0b 44 43 2009-07-10T13:08:05Z Lukasz 2 /* OO Serpentis */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors (more similar to V1647 Ori). f648991d8a49c75bd8c07e17872d02329ac0e45d 45 44 2009-07-10T13:10:15Z Lukasz 2 /* EX Lupis (EXors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors (more similar to V1647 Ori). 005a8cd873905f8c27f2f0dc8798285ef8459d8e 46 45 2009-07-10T13:11:04Z Lukasz 2 /* OO Serpentis */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. 83679e028a042a771cb303aea2a9fcb371490207 6 19 40 2009-07-10T12:24:01Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 20 51 2009-07-10T16:46:15Z Lukasz 2 Created page with 'Dwarf noave have relatively small amplitude outbursts repeating in timescales between days and many years. * Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 ...' wikitext text/x-wiki Dwarf noave have relatively small amplitude outbursts repeating in timescales between days and many years. * Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. [[File:GKPer.png]] 64f555a4189419f09df61ae999f87a84ce7ab306 53 51 2009-07-10T16:48:27Z Lukasz 2 wikitext text/x-wiki Dwarf noave have relatively small amplitude outbursts repeating in timescales between days and many years. * Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. [[File:GKPer.png|200px|thumb|left|AAVSO lightcurve of outbursts of dwarf nova GK Per since 1954]] 4c7fc181538cc96f2a175d6346c9a3098e9755e4 54 53 2009-07-10T16:48:41Z Lukasz 2 wikitext text/x-wiki Dwarf noave have relatively small amplitude outbursts repeating in timescales between days and many years. * Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. [[File:GKPer.png|400px|thumb|left|AAVSO lightcurve of outbursts of dwarf nova GK Per since 1954]] 98453069ea2eb861886206ab6073c0888f420e03 6 21 52 2009-07-10T16:46:35Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 22 55 2009-07-10T17:11:13Z Lukasz 2 Created page with ' * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82|300pix|thumb|left|Ampitude distri...' wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82|300pix|thumb|left|Ampitude distribution for Stripe82 flares.]] bc6b5a4b50a885ccd5c3aa89fe1e2d7fa4a812cb 56 55 2009-07-10T17:11:41Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|300pix|thumb|left|Ampitude distribution for Stripe82 flares.]] cab11b0817815370b9e35b908b409be7a6a16276 58 56 2009-07-10T17:12:14Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|450pix|thumb|left|Ampitude distribution for Stripe82 flares.]] f4a65ae74b3a8c92e659096b732c80d98492bb36 59 58 2009-07-10T17:12:49Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|500pix|thumb|left|Ampitude distribution for Stripe82 flares.]] 89ee7a1651293ec529ed96f06b8294d57d13c7ec 60 59 2009-07-10T17:13:22Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|1500pix|thumb|left|Ampitude distribution for Stripe82 flares.]] 0d8c02a5a75cfdb00104943e31607938131fb03a 61 60 2009-07-10T17:15:02Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|500pix|thumb|left|Ampitude distribution for Stripe82 flares.]] 89ee7a1651293ec529ed96f06b8294d57d13c7ec 6 23 57 2009-07-10T17:11:52Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 24 62 2009-07-13T18:01:47Z Lukasz 2 Created page with 'OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png]] [[File:Be-OGLE-CMD-LMC.png]] [[File:Be-OGLE-ampl.png]] [[File:Be-OGLE-distributions.png]] [[File:B...' wikitext text/x-wiki OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png]] [[File:Be-OGLE-CMD-LMC.png]] [[File:Be-OGLE-ampl.png]] [[File:Be-OGLE-distributions.png]] [[File:Be-OGLE-Type1.png]] [[File:Be-OGLE-Type1-slow.png]] [[File:Be-OGLE-Type2.png]] [[File:Be-OGLE-Type1-2.png]] [[File:Be-OGLE-Type3.png]] [[File:Be-MACHO-modes.png]] [[File:Be-MACHO-mixed-modes.png]] [[File:Be-MACHO-spectra.png]] 79cce008363e403df98bdb02dfe7edcd83316c40 63 62 2009-07-13T18:02:13Z Lukasz 2 wikitext text/x-wiki OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png]] [[File:Be-OGLE-CMD-LMC.png]] [[File:Be-OGLE-ampl.png]] [[File:Be-OGLE-distributions.png]] [[File:Be-OGLE-Type1.png]] [[File:Be-OGLE-Type1-slow.png]] [[File:Be-OGLE-Type2.png]] [[File:Be-OGLE-Type1-2.png]] [[File:Be-OGLE-Type3.png]] [[File:Be-MACHO-modes.png]] [[File:Be-MACHO-mixed-modes.png]] [[File:Be-MACHO-spectra.png]] a5fcc6f4f4c735ee60ae9aaf2a29691d5c66a6a6 76 63 2009-07-13T18:13:19Z Lukasz 2 wikitext text/x-wiki OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png|20pix]] [[File:Be-OGLE-CMD-LMC.png]] [[File:Be-OGLE-ampl.png]] [[File:Be-OGLE-distributions.png]] [[File:Be-OGLE-Type1.png]] [[File:Be-OGLE-Type1-slow.png]] [[File:Be-OGLE-Type2.png]] [[File:Be-OGLE-Type1-2.png]] [[File:Be-OGLE-Type3.png]] [[File:Be-MACHO-modes.png]] [[File:Be-MACHO-mixed-modes.png]] [[File:Be-MACHO-spectra.png]] a55e426f415520d57d16044a403d6436a53ddbd3 77 76 2009-07-13T18:13:55Z Lukasz 2 wikitext text/x-wiki OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png|20px]] [[File:Be-OGLE-CMD-LMC.png]] [[File:Be-OGLE-ampl.png]] [[File:Be-OGLE-distributions.png]] [[File:Be-OGLE-Type1.png]] [[File:Be-OGLE-Type1-slow.png]] [[File:Be-OGLE-Type2.png]] [[File:Be-OGLE-Type1-2.png]] [[File:Be-OGLE-Type3.png]] [[File:Be-MACHO-modes.png]] [[File:Be-MACHO-mixed-modes.png]] [[File:Be-MACHO-spectra.png]] 00f07bf5f931bfadaf8f3040aca6e7e575055bb2 78 77 2009-07-13T18:14:54Z Lukasz 2 wikitext text/x-wiki OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|400px]] d81214fdce4018d7e91960f67b08a08a1bc49c86 79 78 2009-07-13T18:15:32Z Lukasz 2 wikitext text/x-wiki OGLE and MACHO data were studied for Be stars. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] a0912e2cbedfaa81d3075895733ce29a115716e8 80 79 2009-07-13T18:24:15Z Lukasz 2 wikitext text/x-wiki == OGLE and MACHO data were studied for Be stars.== * OGLE (LMC,SMC): [http://ukads.nottingham.ac.uk/abs/2005MNRAS.361.1055S Sabogal et al. 2005], [http://ukads.nottingham.ac.uk/abs/2006A%26A...457..949M Mennickent et al. 2006] * OGLE (Bulge): [http://ukads.nottingham.ac.uk/abs/2008A%26A...478..659S Sabogal et al. 2008] * MACHO: [http://ukads.nottingham.ac.uk/abs/2002AJ....124.2039K Keller et al. 2002] [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] 78e8c2f6d440b003db399681dec7f32621d10e77 6 25 64 2009-07-13T18:02:31Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 26 65 2009-07-13T18:02:49Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 27 66 2009-07-13T18:03:08Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 28 67 2009-07-13T18:03:24Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 29 68 2009-07-13T18:03:43Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 30 69 2009-07-13T18:04:02Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 31 70 2009-07-13T18:04:19Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 32 71 2009-07-13T18:04:35Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 33 72 2009-07-13T18:07:16Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 34 73 2009-07-13T18:08:33Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 35 74 2009-07-13T18:08:52Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 36 75 2009-07-13T18:09:14Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 10 81 27 2009-07-24T09:37:34Z Lukasz 2 wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC_branches%2FCU5%2Fdocs%2Fpersonal%2Flwyrzyko%2Fdocs%2FFluxAlertsManual%2Ffluxalertsmanual.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. == Photometric precision == [[File:Photometric_precision.jpg]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. 69c778ef9615c195f29b6d51f1959b98606d6c73 83 81 2009-07-24T09:39:01Z Lukasz 2 /* Photometric precision */ wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC_branches%2FCU5%2Fdocs%2Fpersonal%2Flwyrzyko%2Fdocs%2FFluxAlertsManual%2Ffluxalertsmanual.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. == Photometric precision == [[File:Photometric_precision.png]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. 1245df7be117e0239a1292c47c0cddf2b2b23f06 84 83 2009-07-24T09:39:50Z Lukasz 2 /* Photometric precision */ wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC_branches%2FCU5%2Fdocs%2Fpersonal%2Flwyrzyko%2Fdocs%2FFluxAlertsManual%2Ffluxalertsmanual.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. 28eddd5132a6581bd44a01a8da92ef7e4faf77f3 6 37 82 2009-07-24T09:38:45Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 8 85 50 2009-07-24T09:47:53Z Lukasz 2 /* Table of transients */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} cbe5b88d83ce052dc10a3ed23a366e7393f728a2 88 85 2009-07-24T09:54:07Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} --- CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png]] 06accacf2f93b4daf57f481e582cdad43b27fcdd 89 88 2009-07-24T09:54:38Z Lukasz 2 /* Table of transients */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|400px]] 804a0349a49ebbfcffddcd0739ba7e1be8a042fe 91 89 2009-07-24T09:55:13Z Lukasz 2 /* CMD of selected variables and transients */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|550px]] 5f37e70c7e46a628cc47081f717fee02168d73ce 92 91 2009-07-24T09:55:27Z Lukasz 2 /* CMD of selected variables and transients */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] eb0e141c9c6f5a5dc8c56488cfe81b2db8a95f57 0 15 86 32 2009-07-24T09:49:42Z Lukasz 2 wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of masive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. a41379a4e52282276e43e8f2efa5f5ec821e8629 6 38 87 2009-07-24T09:50:01Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 39 90 2009-07-24T09:54:48Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 40 93 2009-07-24T12:26:25Z Lukasz 2 Created page with '== Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by S...' wikitext text/x-wiki == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. 51b8a9695c76bde610386e6456c8005c897189ca 95 93 2009-07-27T13:17:59Z Lukasz 2 /* SDSS-II Supernova Survey (Stripe 82) */ wikitext text/x-wiki == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. f476168f45cdfa2ce4edaaa95408e7e044efa020 6 41 94 2009-07-24T12:26:36Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 42 96 2009-07-28T11:08:28Z Lukasz 2 Created page with 'Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. Sour...' wikitext text/x-wiki Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png]] [[File:plot_ews_te_baselinemag.png]] 72228d49cd6b96f618e3c08599bef004956b77e2 99 96 2009-07-28T11:09:58Z Lukasz 2 wikitext text/x-wiki == OGLE == Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] 89200d420daef18641e38ba88b613a6f8f18359f 100 99 2009-07-28T11:21:35Z Lukasz 2 /* OGLE */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|300px]] ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] 212a733acf48dea051a3ccc71c4786d37181020f 6 43 97 2009-07-28T11:08:46Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 44 98 2009-07-28T11:09:05Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 45 101 2009-07-28T11:43:53Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 46 102 2009-07-28T11:44:19Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 103 102 2009-07-28T11:45:25Z Lukasz 2 uploaded a new version of "[[File:Example standard event.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 42 104 100 2009-07-28T11:46:05Z Lukasz 2 /* Exotic events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] abbbf37a68a7202aca3691e7f06dc3c8421b7441 105 104 2009-07-28T11:48:41Z Lukasz 2 /* OGLE's EWS */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png]] 08e09f8594cc2174c6bfc2ba4361fd6f672907d5 107 105 2009-07-28T11:49:39Z Lukasz 2 /* OGLE's EWS */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] 854260277f51539a5ba452b9498161bf4e55b4b4 6 47 106 2009-07-28T11:48:52Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 22 108 61 2009-07-28T12:34:00Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|300px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|500px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] cddbd0a82f3ae9f7fb130f71b6efbd80c7448902 110 108 2009-07-28T12:34:41Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] 5dfcf41a775b9519b90436b658c857ef1872b4d1 111 110 2009-07-28T12:58:57Z Lukasz 2 wikitext text/x-wiki * Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with $\Deta u > 0.7$ mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] 6d35c11c1e16320e5c15b1928749d903df01763f 112 111 2009-07-28T12:59:50Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with $\Deta u > 0.7$ mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] a9468a8f37ea2df6ec0dce77e02c863d9e524666 113 112 2009-07-28T13:00:31Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] 850ec32738272758df273e436f9e735087c3d7f5 114 113 2009-07-28T13:03:23Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] 9a8f6f8607caba9df866e5ddea07bf26780e652e 115 114 2009-07-28T13:05:29Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|300px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] ae12d1b1f72400d2df66a5d0baacf1e1246bcbd6 117 115 2009-07-28T13:06:01Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|400px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] 60a1de6bc66bd966f32942ee74f657d9ac8c7472 6 48 109 2009-07-28T12:34:18Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 49 116 2009-07-28T13:05:38Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 50 118 2009-07-28T13:38:06Z Lukasz 2 Created page with '* there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * amplitude between 6 and 15 mag * quick rise ...' wikitext text/x-wiki * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * amplitude between 6 and 15 mag * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class 4d290cae8a19ef62f976b2da6ae020bdbf8612a2 119 118 2009-07-28T13:46:29Z Lukasz 2 wikitext text/x-wiki * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * amplitude between 6 and 15 mag * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days 97e61c1b2fd90c4013f40c5363f4f24687d7ec54 0 20 120 54 2009-07-28T15:08:40Z Lukasz 2 wikitext text/x-wiki DNe are cataclysmic variable stars consisting of a close binary star system in which one of the components is a white dwarf, which accretes matter from its companion. They are similar to classical novae in that the white dwarf is involved in periodic outbursts, but the mechanisms are different: classical novae result from the fusion and detonation of accreted hydrogen, while current theory suggests that dwarf novae result from instability in the accretion disk, when gas in the disk reaches a critical temperature that causes a change in viscosity, resulting in a collapse onto the white dwarf that releases large amounts of gravitational potential energy[http://en.wikipedia.org/wiki/Dwarf_nova]. * They repeat on irregular intervals of a few weeks to years. * Amplitude up to 6 mag, with <math>A=0.8+1.667 \log(\Delta t_{repeat})</math> * typical DN have two different types of outbursts: more and less energetic. * Classes: U Gem, Z Cam, SU UMa * Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. [[File:GKPer.png|400px|thumb|left|AAVSO lightcurve of outbursts of dwarf nova GK Per since 1954]] b8014825fdcc6fb347440c37b76dde42b6ce7626 0 15 121 86 2009-07-28T17:11:57Z Lukasz 2 wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of masive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. 0145478b52d4411e0d2673466820999e9e980827 0 51 122 2009-07-28T17:16:13Z Lukasz 2 Created page with '[File:figure_rcrb.png]' wikitext text/x-wiki [File:figure_rcrb.png] 01477526949ad024827a5c39accbeab5a6f6108a 123 122 2009-07-28T17:16:32Z Lukasz 2 wikitext text/x-wiki [[File:figure_rcrb.png]] db2f4c3ad63833f22eea9565195ff7a40909d2b9 138 123 2009-07-29T15:37:27Z Lukasz 2 wikitext text/x-wiki Only around 50 known in the Galaxy and Magellanic Clouds. [[File:figure_rcrb.png|400px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] 393cd6a699b5c114f962467c7f82b0f3c40b323d 6 52 124 2009-07-28T17:16:45Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 8 125 92 2009-07-28T17:29:37Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:plot_transients_tau_ampl.png]] [[File:plot_transients_tdecline_ampl.png]] [[File:plot_transients_trise_ampl.png]] [[File:plot_transients_trise_tdecline.png]] d7c419787d5be0b1812e125e1789bc95cb814cc8 130 125 2009-07-29T15:05:12Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:plot_transients_tau_ampl.png]] [[File:plot_transients_tdecline_ampl.png]] [[File:plot_transients_trise_ampl.png]] [[File:plot_transients_trise_tdecline.png]] ba09e23582326ff35d42d69d5c2d63c4428a777e 131 130 2009-07-29T15:05:24Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:plot_transients_tau_ampl.png]] [[File:plot_transients_tdecline_ampl.png]] [[File:plot_transients_trise_ampl.png]] [[File:plot_transients_trise_tdecline.png]] ecebea3846052d48c44fd35e95de526c9871ce33 146 131 2009-07-29T16:33:43Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:LRNs | Luminous Red Novae]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:plot_transients_tau_ampl.png]] [[File:plot_transients_tdecline_ampl.png]] [[File:plot_transients_trise_ampl.png]] [[File:plot_transients_trise_tdecline.png]] 1b871dc2913778438bdb111c1ca12ac6dfa39a3d 148 146 2009-07-29T16:42:16Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:plot_transients_tau_ampl.png]] [[File:plot_transients_tdecline_ampl.png]] [[File:plot_transients_trise_ampl.png]] [[File:plot_transients_trise_tdecline.png]] ecebea3846052d48c44fd35e95de526c9871ce33 149 148 2009-07-29T17:20:11Z Lukasz 2 /* Time scales and amplitudes */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|300px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] ba97a02827e1a3f8e81f88acd7e96cad4929eb56 6 53 126 2009-07-28T17:30:13Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 54 127 2009-07-28T17:30:34Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 55 128 2009-07-28T17:30:55Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 56 129 2009-07-28T17:31:13Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 57 132 2009-07-29T15:22:41Z Lukasz 2 Created page with 'Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Known example: Eta Carinae. [[File:ESO-Eta_Carinae-phot-17a-08-...' wikitext text/x-wiki Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Known example: Eta Carinae. [[File:ESO-Eta_Carinae-phot-17a-08-normal.jpg|200px]] <math>M_V \sim -11 \ldots -8</math> mag * Baseline micro-variability: P around 10-20 days, amplitude 0.1-0.2 mag * "normal eruptions": 1-2 mag (rise within few months), repeating with period of years or decades the brighter abs.mag the shorter period between eruptions) * Giant eruptions ("Eta Carinae type") of around 8 mag, once a few centuries!! * After giant eruption and fade, the star recovers its brightness as the dust disperses. ba9548ed6afe8e1e3b02666deef28d4555f6d8a0 134 132 2009-07-29T15:29:31Z Lukasz 2 wikitext text/x-wiki Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Very heavy stars, often in binary systems, will evolve to W-R stars. Only a few is known. Known example: '''Eta Carinae'''. [[File:ESO-Eta_Carinae-phot-17a-08-normal.jpg|200px|right|thumb|Eta Carinae, ESO]] <math>M_V \sim -11 \ldots -8</math> mag * Baseline micro-variability: P around 10-20 days, amplitude 0.1-0.2 mag * "normal eruptions": 1-2 mag (rise within few months), repeating with period of years or decades the brighter abs.mag the shorter period between eruptions) * Giant eruptions ("Eta Carinae type") of around 8 mag, once a few centuries!! * After giant eruption and fade, the star recovers its brightness as the dust disperses. * Spectroscopic variations with period of 5.5 years (probably due to binarity) * X-ray variability 80df0e9f5d95febdeb95f9ad008217804678bb5a 135 134 2009-07-29T15:31:05Z Lukasz 2 wikitext text/x-wiki Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Very heavy stars(30Msun), often in binary systems, will evolve to W-R stars. Only a few is known. Known example: '''Eta Carinae'''. [[File:ESO-Eta_Carinae-phot-17a-08-normal.jpg|200px|right|thumb|Eta Carinae, ESO]] <math>M_V \sim -11 \ldots -8</math> mag * Baseline micro-variability: P around 10-20 days, amplitude 0.1-0.2 mag * "normal eruptions": 1-2 mag (rise within few months), repeating with period of years or decades the brighter abs.mag the shorter period between eruptions) * Giant eruptions ("Eta Carinae type") of around 8 mag, once a few centuries!! * After giant eruption and fade, the star recovers its brightness as the dust disperses. * Spectroscopic variations with period of 5.5 years (probably due to binarity) * X-ray variability 109dace084e41697f699c7426c50706ffcec1514 136 135 2009-07-29T15:31:22Z Lukasz 2 wikitext text/x-wiki Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Very heavy stars(>30Msun), often in binary systems, will evolve to W-R stars. Only a few is known. Known example: '''Eta Carinae'''. [[File:ESO-Eta_Carinae-phot-17a-08-normal.jpg|200px|right|thumb|Eta Carinae, ESO]] <math>M_V \sim -11 \ldots -8</math> mag * Baseline micro-variability: P around 10-20 days, amplitude 0.1-0.2 mag * "normal eruptions": 1-2 mag (rise within few months), repeating with period of years or decades the brighter abs.mag the shorter period between eruptions) * Giant eruptions ("Eta Carinae type") of around 8 mag, once a few centuries!! * After giant eruption and fade, the star recovers its brightness as the dust disperses. * Spectroscopic variations with period of 5.5 years (probably due to binarity) * X-ray variability 91b39f882727377b60ed18d50b5f56ce5b19ac59 137 136 2009-07-29T15:33:19Z Lukasz 2 wikitext text/x-wiki Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Very heavy stars(>30Msun), often in binary systems, will evolve to W-R stars. Only a few is known. Known example: '''Eta Carinae'''. [[File:ESO-Eta_Carinae-phot-17a-08-normal.jpg|200px|right|thumb|Eta Carinae, ESO]] <math>M_V \sim -11 \ldots -8</math> mag * Baseline micro-variability: P around 10-20 days, amplitude 0.1-0.2 mag * Positioned close to "instability strip", thus the pulsating-like variability * "normal eruptions": 1-2 mag (rise within few months), repeating with period of years or decades the brighter abs.mag the shorter period between eruptions) * Giant eruptions ("Eta Carinae type") of around 8 mag, once a few centuries!! * After giant eruption and fade, the star recovers its brightness as the dust disperses. * Spectroscopic variations with period of 5.5 years (probably due to binarity) * X-ray variability 2b36d081131f05f61bec27ca17cb395c2537ea59 139 137 2009-07-29T15:49:43Z Lukasz 2 wikitext text/x-wiki Known also as S Dor stars. Exhibit slow changes in brightness with occasional outbursts of substantial mass loss. Very heavy stars(>30Msun), often in binary systems, will evolve to W-R stars. Only a few is known. Known example: '''Eta Carinae'''. [[File:ESO-Eta_Carinae-phot-17a-08-normal.jpg|200px|right|thumb|Eta Carinae, ESO]] <math>M_V \sim -11 \ldots -8</math> mag * Baseline micro-variability: P around 10-20 days, amplitude 0.1-0.2 mag * Positioned close to "instability strip", thus the pulsating-like variability * "normal eruptions": 1-2 mag (rise within few months), repeating with period of years or decades the brighter abs.mag the shorter period between eruptions) * Giant eruptions ("Eta Carinae type") of around 8 mag, once a few centuries!! * After giant eruption and fade, the star recovers its brightness as the dust disperses. * Spectroscopic variations with period of 5.5 years (probably due to binarity) * X-ray variability * engine of outbursts is not well understood yet af7dc93bf70a90f0e000b9004f452eb92f5e059d 6 58 133 2009-07-29T15:22:57Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 17 140 36 2009-07-29T16:25:30Z Lukasz 2 wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == '''Please list here any surveys probable to be in operation from 2012 to 2017 suitable for following-up Gaia alerts.''' * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3674069b7a0b196aea12cdacaa939fd5698ddbd0 0 10 141 84 2009-07-29T16:27:54Z Lukasz 2 wikitext text/x-wiki * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. 2b5faaa5cc7748547ea8f1390da95382f5ab2ccc 143 141 2009-07-29T16:30:30Z Lukasz 2 wikitext text/x-wiki == Detection == * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) ---- ---- Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. b14a0541ab081a7d503ab56ee090d879a50c07aa 144 143 2009-07-29T16:31:01Z Lukasz 2 wikitext text/x-wiki == Detection == Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. ---- ---- * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. 6f86feb5376f3ea6bb99715d9b6df770cad9abd3 145 144 2009-07-29T16:31:25Z Lukasz 2 wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. ---- ---- == Detection == * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. e4ae2b423c2dcb82003f545da4c07a01d87f60d5 6 14 142 25 2009-07-29T16:28:55Z Lukasz 2 uploaded a new version of "[[File:Fluxalertsmanual.pdf]]": Updated version of FluxAlerts system manual (GAIA-C5-TN-IOA-LW-002). Valid as of in July 2009. wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 40 147 95 2009-07-29T16:42:01Z Lukasz 2 wikitext text/x-wiki == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading 5c184988288514ab5fbcde8100b7d72f29f9924f 6 59 150 2009-07-29T17:20:27Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 8 151 149 2009-07-29T17:23:33Z Lukasz 2 /* Time scales and amplitudes */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] d936ed99970f64a1600f5f70aab3c179576fd96b 0 9 152 15 2009-08-06T15:48:43Z Gsawgwikiadmin 1 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:Be | Be-type stars]] * [[Triggers:AGN | AGNs]] 8417ea184edc17aa209680ba3c57d65f2f0b9295 153 152 2009-08-06T16:11:30Z Simkoz 10 wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:Be | Be-type stars]] * [[Triggers:AGN | Active Galactic Nuclei (AGNs, Quasars, QSOs)]] 8f8ca3a2a455a13a7fe84c88ee94fa8967bf6aa2 174 153 2009-08-19T10:04:28Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:AGN | Active Galactic Nuclei (AGNs, Quasars, QSOs)]] f1110af1572efdc7803907519c87575092abba1d 0 15 154 121 2009-08-10T09:52:39Z Lukasz 2 /* NGC300-OT */ wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of masive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. 6182aa99d9b92b8d8a76f78c5e1694581ceb7e0e 155 154 2009-08-10T09:56:26Z Lukasz 2 /* NGC300-OT */ wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of masive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. 2bb9ec28acbbb923bdaea7e92e2a9a61b361fc74 156 155 2009-08-10T09:58:29Z Lukasz 2 /* NGC300-OT */ wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of massive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star * no radio or X-ray counterpart detected * no star visible at that location prior to the outburst on HST archival images. [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. 57da28e9524e4d5d56aa8e7000d4fe2ee9c6cf65 175 156 2009-08-24T08:40:07Z Lukasz 2 wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of massive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star * no radio or X-ray counterpart detected * no star visible at that location prior to the outburst on HST archival images. [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. == OT060420 == Very short (~12 min) and bright (~ 5 mag) transient detected by CONCAM all-sky cameras [http://arxiv.org/abs/astro-ph/0607033]. The astronomical nature of the event is disputable, as the detection was made only on two out of three telescopes. One explanation is that the transient was variable. Gaia will be able to detect such transients and also provide per-ccd photometry, every 4 seconds. d38a07ff5ddaa6091b0f0412edc7b7c280628b44 0 40 157 147 2009-08-10T14:03:44Z Gaia 3 /* Supernovae type Ia */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576) {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 | |- | Ib | 7000 | |- | IIL | 5600*f | |- | IIP | 28500*(1-f) | |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading d0606807ffb5f9d770f600141d5dd11b223c44be 158 157 2009-08-10T14:12:05Z Gaia 3 /* Supernovae type Ia */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576) {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 5600*f |- | IIP | 28500*(1-f) |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading ba8f7bad33519e328526b0bb9ec51bd194600bc5 159 158 2009-08-10T14:20:51Z Gaia 3 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type. The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 5600*f |- | IIP | 28500*(1-f) |- |} The other piece of information needed is the Luminosity function == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading ef9f3832e0eb591e5e81551d914cfbe9b0487dec 160 159 2009-08-10T14:27:17Z Gaia 3 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type. The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 5600*f |- | IIP | 28500*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! M\dG\u ! sigma\dG\u |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading 63e29d14357c09a58686410c9be5a94a66187925 162 160 2009-08-10T14:30:02Z Gaia 3 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type. The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 5600*f |- | IIP | 28500*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</match> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading ea86aea12d1eda0addccef425a546d13ac5174db 163 162 2009-08-10T14:30:51Z Gaia 3 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type. The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 5600*f |- | IIP | 28500*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading 09d3cb6cd2eb1424e536bafb9c61a202c8e9dc32 164 163 2009-08-10T14:33:59Z Gaia 3 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 5600*f |- | IIP | 28500*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading 3cf4c1bc234145c953b004774e569ed59d845389 165 164 2009-08-10T14:35:45Z Gaia 3 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading 4832fffe939ff265562d3c7f22a82a566c52fbdb 173 165 2009-08-19T10:03:44Z Lukasz 2 wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] 702cf189a478c57cd75f0067eca347f8785d9c1f 8 3 161 19 2009-08-10T14:27:27Z Gsawgwikiadmin 1 wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** other surveys|Other surveys * SEARCH * TOOLBOX 3cf698d566426703b4e68ea67217891f5756a4a4 0 60 166 2009-08-10T14:44:37Z Gsawgwikiadmin 1 Created page with 'Links and information on current and future photometric and astrometric surveys: * [http://www.lpl.arizona.edu/css/ Catalina Real-Time Transient Survey], [http://ukads.nottingha...' wikitext text/x-wiki Links and information on current and future photometric and astrometric surveys: * [http://www.lpl.arizona.edu/css/ Catalina Real-Time Transient Survey], [http://ukads.nottingham.ac.uk/abs/2009ApJ...696..870D Drake et al. 2009] * [http://www.astro.caltech.edu/~george/pq/ Palomar-Quest], [http://ukads.nottingham.ac.uk/abs/2008AN....329..263D Djorgovski et al. 2008] * All Sky Automated Survey ([http://www.astrouw.edu.pl/asas/ ASAS]), [http://ukads.nottingham.ac.uk/abs/2002AcA....52..397P Pojmanski 2002], limited by V~14 mag, all sky survey, observing from Chile since 1997 and from Hawai since 2006. * Optical Gravitational Lensing Experiment ([http://ogle.astrouw.edu.pl OGLE]), [http://adsabs.harvard.edu/abs/2003AcA....53..291U Udalski 2003], Bulge, LMC and SMC only, continuously gathers data since 1996. * SDSS-II Supernova Survey, e.g. Holtzman et al. 2008 * Palomar Transient Factory, e.g. Rau et al. 2009, in operation since Dec.2008 a54e2748da63a72948c10bdaa181109005951674 0 42 167 107 2009-08-10T15:06:41Z Gsawgwikiadmin 1 wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.gif|thumb|300pix|Light curve of GSC 3656-1328 microlensing event]] af3992dac7fdf10573168bbfa1a45086c6683ce9 168 167 2009-08-10T15:07:02Z Gsawgwikiadmin 1 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.gif|left|thumb|300pix|Light curve of GSC 3656-1328 microlensing event]] 402e6080d96fd21dccfda3fefc97758ed492fac7 170 168 2009-08-10T15:08:10Z Gsawgwikiadmin 1 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300pix|Light curve of GSC 3656-1328 microlensing event]] fbb4a23b310a7654fdf77655010528dbbb1f578f 171 170 2009-08-10T15:08:21Z Gsawgwikiadmin 1 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|400pix|Light curve of GSC 3656-1328 microlensing event]] 640eae20cd5eefa618df6ce8b2879ff2b352ba22 172 171 2009-08-10T15:08:31Z Gsawgwikiadmin 1 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] 307891c8ed6464ae0d0d2477eaeefd2108a15a51 6 61 169 2009-08-10T15:07:50Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 51 176 138 2009-08-24T13:31:33Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == Only around 50 known in the Galaxy and Magellanic Clouds. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 8 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline [[File:figure_rcrb.png|400px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] == DY Persei == Some people claim it is a similar type to RCrB, however the drops in magnitude are much smaller and seem to be periodical (P~1000d). [[File:DYPer.png|400px|left|thumb|Example light curve of DY Per-type candidate]] ef0aded282fd2f6e42d7a074ea0437170c53bb3d 177 176 2009-08-24T13:32:05Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 8 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline == DY Persei == [[File:DYPer.png|400px|left|thumb|Example light curve of DY Per-type candidate]] Some people claim it is a similar type to RCrB, however the drops in magnitude are much smaller and seem to be periodical (P~1000d). 1415e660b5cb145a12f5db57db4fb74a0f26c536 180 177 2009-08-24T13:33:54Z Lukasz 2 /* DY Persei */ wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 8 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline == DY Persei == [[File:DYPer.png|400px|right|thumb|Example OGLE light curve of DY Per-type candidate]] Some people claim it is a similar type to RCrB, however the drops in magnitude are much smaller and seem to be periodical (P~1000d). ce30a226fba1d28cec743525423313bbdad108df 181 180 2009-08-24T13:34:07Z Lukasz 2 /* DY Persei */ wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 8 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] Some people claim it is a similar type to RCrB, however the drops in magnitude are much smaller and seem to be periodical (P~1000d). ecd32664c8e6dd0706d85cf3c5ad3cb0cccd2c3f 6 62 178 2009-08-24T13:33:04Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 63 179 2009-08-24T13:33:21Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 64 182 2009-08-25T21:08:45Z Simkoz 10 Created page with '== Active Galactic Nuclei (AGNs) == '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy...' wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The energy radiated from the central engine is produced by accretion of matter onto the black hole. The emission from AGNs is observed at all wavelengths. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their aperiodic variability with an amplitude of 0.5 magnitude in I-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(V-I)<1.0 mag. '''Spatial distribution:''' There are approximately 1, 4 and 40 AGNs per square degree brighter than I<16, 18 and 20 mag, respectively. dc4e7517e19cd3a7469dc53ff1a18602ae80c6c2 183 182 2009-08-25T21:18:47Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The energy radiated from the central engine is produced by accretion of matter onto the black hole. The emission from AGNs is observed at all wavelengths. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an amplitude of 0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. 456f78fb4ac96654a2d750148c28b70dcdcb5fde 184 183 2009-08-26T13:58:56Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a broader term for a group of objects such as: quasars, QSOs, Serfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects, where the latter ones are represented by Seyfert 1 and Seyfert 2 galaxies. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an average amplitude of ~0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. 8e53cdd3b04e6677a5e0744a836aba797a865920 185 184 2009-08-26T14:00:11Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a broader term for a group of objects such as: quasars, QSOs, Serfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an average amplitude of ~0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. 0a319dad431ba6c4f734bb4428a1029173cce58d 186 185 2009-08-26T14:28:21Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an average amplitude of ~0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Exemplary light curves of quasars:''' [[File:Example.jpg]] 088ff67fe50970473fedc8e481a67734b1a1e61a 188 186 2009-08-26T14:30:05Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an average amplitude of ~0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Exemplary light curves of quasars:''' [[File:AGN_lc.jpg]] 11383dc3299c4e14b43097af5bf1ddc0f0671e84 189 188 2009-08-26T14:30:47Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an average amplitude of ~0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Exemplary light curves of quasars:''' [[File:AGN_lc.jpg]] 8312fd97a613e5a30b9c0236e42316ecd94f7c2c 190 189 2009-08-26T14:32:21Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' In the optical part of the spectrum, AGNs are characterized by their long-term aperiodic variability with an average amplitude of ~0.5 magnitude in ''I''-band. Majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Exemplary light curves of quasars:''' [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] 7a1ac246c869739a7d798e230fc1045aa47af15c 191 190 2009-08-26T14:39:03Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' The majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Exemplary light curves of quasars:''' [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] 626365c0d0780af3e08ee5d4c37506f58fe55973 192 191 2009-08-26T14:54:14Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' The majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Exemplary light curves of quasars:''' [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] '''Quasars on a color-magnitude diagram (CMD):''' [[File:AGN_cmd.jpg|300px|thumb|left|Quasars on a CMD]] 42b5ead0127ac443133ce005ec589cf535944063 194 192 2009-08-26T15:01:57Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high and low luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' The majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. == Exemplary light curves of quasars and their location on a CMD == [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] [[File:AGN_cmd.jpg|300px|thumb|left|Quasars on a CMD]] <br /> [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] 920d73b78bbc530ed24d6412feec630d2631cd61 195 194 2009-08-26T15:09:04Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V<-23 mag) and low (M_V>-23 mag)luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' The majority of AGNs up to a redshift of z<2.6 occupy colors of 0.4<(''V-I'')<1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. == Exemplary light curves of quasars and their location on a CMD == [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] [[File:AGN_cmd.jpg|300px|thumb|left|Quasars on a CMD]] <br /> [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] b75679dcdbf064c5fe902112d068b226c417374b 196 195 2009-08-26T15:09:41Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V < -23 mag) and low (M_V > -23 mag) luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T=R^{-3/4}</math> (and <math>R=\lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' The majority of AGNs up to a redshift of z < 2.6 occupy colors of 0.4 < (''V-I'') < 1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. == Exemplary light curves of quasars and their location on a CMD == [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] [[File:AGN_cmd.jpg|300px|thumb|left|Quasars on a CMD]] <br /> [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] 6bc21ad1f48ad27e599c58e239cd0579dde4fdbd 197 196 2009-08-26T15:11:31Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V < -23 mag) and low (M_V > -23 mag) luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T \propto R^{-3/4}</math> (and <math>R \propto \lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. '''Optical appearance:''' The majority of AGNs up to a redshift of z < 2.6 occupy colors of 0.4 < (''V-I'') < 1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. == Exemplary light curves of quasars and their location on a CMD == [[File:AGN_lc.jpg|300px|thumb|left|Exemplary light curves of quasars]] [[File:AGN_cmd.jpg|300px|thumb|left|Quasars on a CMD]] <br /> [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] 5b87b1ef9b83e30e44645ac91ebee4cabf7400a9 198 197 2009-08-26T15:19:46Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == [[File:AGN_lc.jpg|300px|thumb|Exemplary light curves of quasars]] (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V < -23 mag) and low (M_V > -23 mag) luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T \propto R^{-3/4}</math> (and <math>R \propto \lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. [[File:AGN_cmd.jpg|300px|thumb|Quasars on a CMD]] '''Optical appearance:''' The majority of AGNs up to a redshift of z < 2.6 occupy colors of 0.4 < (''V-I'') < 1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I''<16, 18 and 20 mag, respectively. '''Links:''' [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] 7ece3e8eba743fdfc6e669c67c04cacd85277e86 199 198 2009-08-26T15:28:41Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == [[File:AGN_lc.jpg|300px|thumb|Exemplary light curves of quasars]] (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V < -23 mag) and low (M_V > -23 mag) luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T \propto R^{-3/4}</math> (and <math>R \propto \lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. [[File:AGN_cmd.jpg|300px|thumb|Quasars on a CMD]] '''Optical appearance:''' The majority of AGNs up to a redshift of z < 2.6 occupy colors of 0.4 < (''V-I'') < 1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution on the sky:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I'' < 16, 18 and 20 mag, respectively. '''Links:''' [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] d6a24e1d645c209aa116ac8998083f67a6d72696 200 199 2009-08-26T15:30:54Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == [[File:AGN_lc.jpg|300px|thumb|Exemplary light curves of quasars]] (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V < -23 mag) and low (M_V > -23 mag) luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T \propto R^{-3/4}</math> (and <math>R \propto \lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. [[File:AGN_cmd.jpg|300px|thumb|Quasars on a CMD of the Large Magellanic Cloud]] '''Optical appearance:''' The majority of AGNs up to a redshift of z < 2.6 occupy colors of 0.4 < (''V-I'') < 1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.5 magnitude in ''I''-band. '''Spatial distribution on the sky:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I'' < 16, 18 and 20 mag, respectively. '''Links:''' [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] 4f90f84ce23ad58f9f97c2c11ba1206dbfcfb173 6 65 187 2009-08-26T14:29:06Z Simkoz 10 OGLE-III light curves of AGNs wikitext text/x-wiki OGLE-III light curves of AGNs f8c90827f47683f3e3dc8706bd71a22b2b8b8cf7 6 66 193 2009-08-26T14:54:41Z Simkoz 10 Quasars on a CMD wikitext text/x-wiki Quasars on a CMD 6afac2bebddc39ae2220a37533acba69db6a1629 0 64 201 200 2009-08-26T15:33:08Z Simkoz 10 wikitext text/x-wiki == Active Galactic Nuclei (AGNs) == [[File:AGN_lc.jpg|300px|thumb|Exemplary light curves of quasars]] (AGN is a term for a broader group of objects including: quasars, quasi-stellar objects (QSOs), Seyfert 1/2 galaxies, blazars, etc.) '''AGNs:''' They are cosmologically distant sources, that can be used for fixing reference frames for studying motions of stars in the Galaxy and in the nearby galaxies within the Local Group. The majority of AGNs would be the most energetic objects in the Universe. A widely accepted model for active galactic nuclei nowadays is that their emission is caused by the release of gravitational energy during accretion of matter onto super-massive black holes residing in the very centers of galactic nuclei. Following the unified model of AGNs, we can crudely divide them into high (M_V < -23 mag) and low (M_V > -23 mag) luminosity objects. In the high luminosity AGNs emission comes either from the jet of relativistic matter pointing towards the observer (blazars), from the vicinity of the nucleus (QSOs) or from both. The observed optical variability in these objects, if present, has the shortest characteristic time-scales of days or weeks, what puts an upper limit on the size of the emission region, ie., r < 0.01 pc or approximately r < 10^16 cm. Low luminosity AGNs depending on the inclination angle of the accretion disk are Seyfert 1 if the disk is close to face-on or Seyfert 2 if it closer to edge-on. The face-on position allows to directly probe the very inner region of the AGNs -- the accretion disk (and Broad emission Line Region). This is where the most energetic radiation originates from, including X-ray, UV flux and optical continuum. Once the inclination angle of the disk changes from face-on to the edge-on, the dust torus begins to obscure the accretion disk as well as the Broad emission Line Region (BLR). Part of the emitted light is then being absorbed by the dust torus and re-radiated in a form of thermal radiation at longer, infrared wavelengths. '''Spectra:''' The spectra of AGNs are often roughly divided into a `blue bump' and an `infrared bump'. Emission at short wavelengths is caused by an optically thin accretion disk radiating with a power-laws <math>T \propto R^{-3/4}</math> (and <math>R \propto \lambda^{4/3}</math>). Dust grains evaporate above ~2000 K, what corresponds to a local minimum at <math>\lambda=1 \mu</math>m in the AGNs spectral energy distributions (SEDs). The `infrared bump', for wavelengths longer than 1 <math>\mu</math>m, is believed to be a fingerprint of hot dust re-radiating more energetic radiation. [[File:AGN_cmd.jpg|300px|thumb|Quasars on a CMD of the Large Magellanic Cloud]] '''Optical appearance:''' The majority of AGNs up to a redshift of z < 2.6 occupy colors of 0.4 < (''V-I'') < 1.0 mag. The characteristic long-term aperiodic variability of AGNs, in the optical part of the spectrum, has an average amplitude of ~0.3 magnitude in ''I''-band. '''Spatial distribution on the sky:''' There are approximately 0.4, 4 and 40 AGNs per square degree brighter than ''I'' < 16, 18 and 20 mag, respectively. '''Links:''' [http://astro.ia.uz.zgora.pl/~simkoz/projects/AGN_MC/database/ Database of Quasars Behind the Magellanic Clouds] a64b3488c57ecdbbb31d0388d0893a8165bfee2c 0 42 202 172 2009-08-26T17:39:25Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|left|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8.]] 0454a454a902c61c3eec21ff52e2b2b06f20bdd4 204 202 2009-08-26T17:40:16Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|left|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 down to V=18 mag.]] 6aca7ea739de4df5e7c463b5f6a48f99d992b916 205 204 2009-08-26T17:40:29Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|left|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] ded463a9da94c51daf841076ec36e8c148052d95 206 205 2009-08-27T11:37:51Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|right|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|left|thumb|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] 297993267c18ad6f6834e756feff46703aef2919 208 206 2009-08-27T11:43:37Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|right|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|left|thumb|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge and about 750 over all sky. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days.]] 36cd9fa70a7721c378f70ef48c143c4162031d60 211 208 2009-08-27T11:44:47Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|right|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|left|thumb|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge and about 750 over all sky. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days.]] 7c18a531e699b3d573c8d9e6d944d3b868395659 212 211 2009-08-27T11:45:14Z Lukasz 2 /* All-sky events */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|right|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|left|thumb|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] == Detection efficiency for Gaia == Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge and about 750 over all sky. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days.]] 9bea9d191104a6cd494e1f893a4d5c390b3e7b1d 213 212 2009-08-27T11:45:34Z Lukasz 2 wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|left|thumb|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|right|thumb|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|left|thumb|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- == Detection efficiency for Gaia == Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge and about 750 over all sky. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days.]] d5d455e3ce00642155e88957cc0deafe8540507d 214 213 2009-08-27T11:48:10Z Lukasz 2 wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- === Detection efficiency for Gaia === Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge and about 750 over all sky. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days.]] 4d89ab1fa93e9878fb11afb7387616a90efc51bb 215 214 2009-08-27T11:49:10Z Lukasz 2 /* Detection efficiency for Gaia */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- === Detection efficiency for Gaia === Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge and about 750 over all sky. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days. For detections before the peak.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days. For detections before the peak.]] 814cacf6bebf36c18fdaa8fec8fa2550fe444434 227 215 2009-08-27T15:23:54Z Lukasz 2 /* Detection efficiency for Gaia */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- === Detection efficiency for Gaia === Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge. Assuming mean time-scale of 30 days and mean detection efficiency for events before the peak of 30%, it means about a 1000 events towards the Bulge should be detected by Gaia. Over entire sky there is something like 750 events expected to happen during the mission. If the mean time-scale is about 15 days, the mean efficiency is about 20%, thus there should be additional 150 events detected all over the sky before they reach the peak brightness. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days. For detections before the peak.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days. For detections before the peak.]] e17a8b193a5fa586399b1ab9fc8562ef4f83b317 228 227 2009-08-27T15:25:58Z Lukasz 2 /* Detection efficiency for Gaia */ wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- === Detection efficiency for Gaia === Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge. Assuming mean time-scale of 30 days and mean detection efficiency for events before the peak of 30%, it means about a 1000 events towards the Bulge should be detected by Gaia. This number, however, might be affected by crowding effects in the Bulge. On the other hand, the satellite is planned to be slowed down a bit to observe Baade's Window (towards the Bulge) more frequently, what can increase the efficiency of detection. Over entire sky there is something like 750 events expected to happen during the mission. If the mean time-scale is about 15 days, the mean efficiency is about 20%, thus there should be additional 150 events detected all over the sky before they reach the peak brightness. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days. For detections before the peak.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days. For detections before the peak.]] c0dfd592c3959fd8eeeb7244eafbf9e784265674 6 67 203 2009-08-26T17:39:44Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 68 207 2009-08-27T11:38:16Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 69 209 2009-08-27T11:43:55Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 70 210 2009-08-27T11:44:11Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 22 216 117 2009-08-27T13:25:08Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|400px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky|500px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. fd5b6c9a83340d53c1119bb0ead0074d9a94c5a5 217 216 2009-08-27T13:28:05Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|400px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|500px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 07153c49dfbbe630a5db8d822cb6d639993c17a1 219 217 2009-08-27T13:32:01Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|400px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 0efa4f4bcbc0fd2b48a1a1ce00b2080056aa5ca2 6 71 218 2009-08-27T13:28:21Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 72 220 2009-08-27T13:32:15Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 221 220 2009-08-27T13:35:32Z Lukasz 2 uploaded a new version of "[[File:FlareGJ3331A-PioftheSky.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 8 222 151 2009-08-27T13:46:48Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 72fe65199b9ff639848fe3654f7a1c093dad3621 249 222 2009-10-06T09:43:08Z Lukasz 2 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 53ae148d95de56b8584ad793e376500b270418dd 0 73 223 2009-08-27T14:07:21Z Lukasz 2 Created page with 'Very short-lived optical transients associated with enormous gamma-ray outbursts. * time-scales from seconds to minutes * in maximum can reach up to 5 mag, but the whole range o...' wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. * time-scales from seconds to minutes * in maximum can reach up to 5 mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] [[File:GRB08-PI.png|400px]] c413239946b9ac2d3292da2d80a513867f6a5bac 226 223 2009-08-27T14:08:52Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. * time-scales from seconds to minutes * in maximum can reach up to 5 mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] 3b17f0ebdd9bad261e0d0061ff9fbe8748745f2c 229 226 2009-08-28T11:35:18Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] c3e092bad1c91849ec0ef47a73169f3fe031d3bf 230 229 2009-08-28T13:37:03Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] 1a5ce5b86b678c2bac10c38070923d27965913aa 234 230 2009-09-07T15:39:27Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] Only about 1 per cent of GRBs are detectable by Gaia. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. If we also demand the transient to be visible in the second FOV (after 105 min), the efficiency drops dramatically. 3d1f3ecb435da16040ce98b1bc80b2123b37d51e 236 234 2009-09-07T15:40:17Z Lukasz 2 /* Detecting GRBs with Gaia */ wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] Only about 1% of GRBs is detectable by Gaia. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. If we also demand the transient to be visible in the second FOV (after 105 min), the efficiency drops dramatically. 8fb00c3a16411d8086776794894cf21b9690e1aa 237 236 2009-09-08T12:32:20Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] Only about 1% of GRBs is detectable by Gaia. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. If we also demand the transient to be visible in the second FOV (after 105 min), the efficiency drops dramatically. 79267a36c7098962a20e7381f593b1c125ff4361 238 237 2009-09-08T12:35:44Z Lukasz 2 /* Detecting GRBs with Gaia */ wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] Only about 1% of GRBs is detectable by Gaia. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. If we also demand the transient to be visible in the second FOV (after 105 min), the efficiency drops dramatically. [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] dbad3d6159443c97acb6f8e1547641b63ee18027 240 238 2009-09-08T12:44:51Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB-schematic_lightcurve.png|300px]] from Piran, 2005. [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] Only about 1% of GRBs is detectable by Gaia. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. If we also demand the transient to be visible in the second FOV (after 105 min), the efficiency drops dramatically. [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] 9cf290b5322c2e952db711e668a0b8b396230ab5 244 240 2009-09-09T08:11:20Z Lukasz 2 /* Detecting GRBs with Gaia */ wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB-schematic_lightcurve.png|300px]] from Piran, 2005. [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] Only about 3-5% of GRBs is detectable by Gaia. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] d08fc73d8be50273ba709e44018abc481ff1c6a0 245 244 2009-09-10T09:29:22Z Lukasz 2 wikitext text/x-wiki Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB-schematic_lightcurve.png|300px]] from Piran, 2005. [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] d1c00173b374de198d43efda3df40c177ed23cc5 6 74 224 2009-08-27T14:07:37Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 75 225 2009-08-27T14:07:54Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 9 231 174 2009-09-07T14:46:06Z Thomas.lebzelter 12 /* Possible triggers for Science Alerts */ long period variables added wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:Be | Long period variables]] * [[Triggers:AGN | Active Galactic Nuclei (AGNs, Quasars, QSOs)]] dba55dcaccd88a00efcb3ded333f2a6bf9b5866e 232 231 2009-09-07T14:46:29Z Thomas.lebzelter 12 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:LPVs | Long period variables]] * [[Triggers:AGN | Active Galactic Nuclei (AGNs, Quasars, QSOs)]] 97446da2f8ac889328d5838a037878862de72828 0 76 233 2009-09-07T15:04:40Z Thomas.lebzelter 12 Description of LPVs entered - first version wikitext text/x-wiki Long period variables (LPVs) LPVs are a class of variability characteristic for evolved stars of low and intermediate mass. Most of them are on the Asymptotic Giant Branch (AGB). Being intrinsically very luminous Gaia will measure them in a large space volume. The LPV type variability is characterized by light variations reaching an amplitude of up to 6 mag in the visual range, but also stars with light amplitudes below 1 mag belong to this group. They all show light variations on time scales between 30 and 1000 days mixed with phases of irregularity. For the Gaia Science Alert system the critical case is a subgroup, normally dubbed "miras", with amplitudes of several magnitudes and periods of a few hundred days. Due to their large amplitudes some of these stars will fall below the Gaia detection limit during their light minimum. When the star's brightness rises again, it would suddenly appear in the Gaia field as a "new" star and might trigger a science alert, especially as the star may continue to increase in brightness for several weeks. Possible strategies to identify such events: first, these stars are very red. Including a colour criterion may help to identify these targets. Typical effective temperature is below 4000 K (corresponding BP-RP colours have to be added later). Once the star has been processed by the variability analysis (CU7) a check of the variability class should avoid any further misinterpretation (i.e. problem occurs only at the first detection). Finally, the increase in brightness is comparably slow - about 1 mag in 25 days, although there are also cases known with a very steep increase in brightness (highly asymmetric light curve). bf2d63b042519b5badcc26de80bb972e3ab677b0 6 77 235 2009-09-07T15:39:43Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 242 235 2009-09-09T08:09:37Z Lukasz 2 uploaded a new version of "[[File:Plot grb eff.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 243 242 2009-09-09T08:10:13Z Lukasz 2 uploaded a new version of "[[File:Plot grb eff.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 78 239 2009-09-08T12:35:57Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 79 241 2009-09-08T12:45:06Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 40 246 173 2009-09-22T20:39:24Z Gsawgwikiadmin 1 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] 507a55e2fff1509b4b0a9281b91a71ed919863b1 8 3 247 161 2009-10-02T16:14:16Z Gsawgwikiadmin 1 added Monitoring to Alerts Sidebar wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * SEARCH * TOOLBOX 16a36a37c16111b6bd41924165818c0ef16bbbc1 0 80 248 2009-10-02T16:16:43Z Gsawgwikiadmin 1 Created page with 'Gaia Science Alerts will also provide an opportunity for continuous monitoring of selected objects. Targets can be added or removed anytime during the mission.' wikitext text/x-wiki Gaia Science Alerts will also provide an opportunity for continuous monitoring of selected objects. Targets can be added or removed anytime during the mission. b709b209ffc081203840f67996bb3cbe64256634 0 81 250 2009-10-06T09:58:00Z Lukasz 2 Created page with 'There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular interv...' wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. [Figure: CV-VYScl.png] 0836f37e18a175d5c7ccc5ab70cb447c385f1d7d 0 81 251 250 2009-10-06T09:58:14Z Lukasz 2 wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. [[Figure: CV-VYScl.png]] af77d43b8886b3393448e797bc7fe08943da8398 252 251 2009-10-06T09:58:41Z Lukasz 2 wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. [[File:CV-VYScl.png]] 61bbe6377d1a714ade3902e4b324a4d42c2de927 254 252 2009-10-06T10:00:12Z Lukasz 2 /* VY Sculptoris */ wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. 76991d2d9f1b883f951266efc5b60fcfcfe87aaa 255 254 2009-10-06T10:02:31Z Lukasz 2 /* VY Sculptoris */ wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). It is suspected these are supersoft X-ray binaries, containing a WD. [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. bad57ada76ed6497c5cffa84993dae8efcc72a58 256 255 2009-10-06T10:05:26Z Lukasz 2 /* VY Sculptoris */ wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. * V504 Cen has period of 4.21h ec0351a2a26de844e8107b2f32541551e6685574 257 256 2009-10-06T10:07:00Z Lukasz 2 /* VY Sculptoris */ wikitext text/x-wiki There is a very large variety of behaviours of CVs. == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. * V504 Cen has period of 4.21h and went down by 6 mag in 2006 and remained in it for nearly a year. 33fb15e6d053896510007b0c87e6751862b62ce7 6 82 253 2009-10-06T09:59:08Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 77 258 243 2009-10-06T16:26:20Z Lukasz 2 uploaded a new version of "[[File:Plot grb eff.png]]": Efficiency for mag1=15.0 mag GRBs. wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 73 259 245 2009-10-06T16:27:51Z Lukasz 2 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag.png|200px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] 6eb7760eb037beb31ce61179401a30f3b2178a4f 261 259 2009-10-06T16:34:51Z Lukasz 2 /* Detecting GRBs with Gaia */ wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] 39bf7c5134daca6ff798dd294476131435247966 262 261 2009-10-06T16:36:11Z Lukasz 2 /* Detecting GRBs with Gaia */ wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] 69b19ed63c91114a5f21a73e25703f869584a1a2 6 83 260 2009-10-06T16:28:34Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 84 263 2009-10-06T16:36:34Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 22 264 219 2009-10-09T12:39:24Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|400px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 1d7034c433d9c4a0e081efd346b86349b06a7157 265 264 2009-10-09T13:01:50Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|right]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Flare_example_Stripe82.png|400px]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. e36ab6be2b3a20e77aee635fee5f2cf181bdb9d1 267 265 2009-10-09T13:02:45Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 63ca0650f093e7c51bd24a48fb67f20e401573ff 268 267 2009-10-09T13:03:07Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. f6619499f24c5f1819b5d10494de3a67478ff5ea 269 268 2009-10-09T14:16:28Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. d3d2a69fdac8318baa06ea65ab6ae97f6c522420 6 85 266 2009-10-09T13:02:13Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 51 270 181 2009-10-12T12:54:50Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline RCrB can be distinguished from other Red Giants based on the fact that an RCB’s circumstellar shell seem thinner than that of most common AGB stars [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009]. == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). 14ef4526a07d2c2a81d532903efdc829114dacd6 271 270 2009-10-12T12:55:07Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline RCrB can be distinguished from other Red Giants based on the fact that an RCB’s circumstellar shell seem thinner than that of most common AGB stars [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009]. TBC... == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). cdb99964035364b781d5f43b2720a34e66c8af79 275 271 2009-10-12T13:44:32Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009] Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline * fading rate: 0.04 mag/day * absolute magnitude range: M_V=-5.2 to -3.4 mag * 0 < V-I < 2 * near-infrared excess: between 0 and 3 in J-H and H-K [[File:RCRB-nearIR.png|500px] == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). * their distributions match those of typical carbon stars (type N) * fading rate: 0.01 mag/day * absolute magnitude range: M_V=-3 to -1.8 mag * V-I > 1.5 ee8433afa9065116b18a5926c867644d8b4d75bb 276 275 2009-10-12T13:44:51Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009] Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline * fading rate: 0.04 mag/day * absolute magnitude range: M_V=-5.2 to -3.4 mag * 0 < V-I < 2 * near-infrared excess: between 0 and 3 in J-H and H-K [[File:RCRB-nearIR.png|500px]] == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). * their distributions match those of typical carbon stars (type N) * fading rate: 0.01 mag/day * absolute magnitude range: M_V=-3 to -1.8 mag * V-I > 1.5 611e9305b93c7cd820f50905d0aa0f388a810bf2 279 276 2009-10-12T13:46:24Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009] Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline * fading rate: 0.04 mag/day * absolute magnitude range: M_V=-5.2 to -3.4 mag * 0 < V-I < 2 * near-infrared excess: between 0 and 3 in J-H and H-K [[File:RCRB-nearIR.png|700px]] == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). * their distributions match those of typical carbon stars (type N) * fading rate: 0.01 mag/day * absolute magnitude range: M_V=-3 to -1.8 mag * V-I > 1.5 ee87af0f51b94fe84a11c58f372194b1a6abcafe 284 279 2009-10-26T17:59:55Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich and hydrogen-deficient evolved F and G supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009]. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline * fading rate: 0.04 mag/day * absolute magnitude range: M_V=-5.2 to -3.4 mag * 0 < V-I < 2 * near-infrared excess: between 0 and 3 in J-H and H-K [[File:RCRB-nearIR.png|700px]] == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). * their distributions match those of typical carbon stars (type N) * fading rate: 0.01 mag/day * absolute magnitude range: M_V=-3 to -1.8 mag * V-I > 1.5 c5739402628fa80738747d847aecf558a1269f35 0 10 272 145 2009-10-12T12:56:56Z Lukasz 2 wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. ---- ---- == Detection == * '''Currently, the detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter * '''In the future it will also use:''' ** accumulated BP and RP colours ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 95aa3492759ef64862c4516b208fea7ef0783639 0 86 273 2009-10-12T13:00:00Z Lukasz 2 Created page with 'List of catalogues to be used for cross-matching Gaia Science Alerts sources: * SDSS * 2MASS * NED * ASAS * OGLE * INTEGRAL [http://arxiv.org/abs/0910.1704] - Gamma-ray sources,...' wikitext text/x-wiki List of catalogues to be used for cross-matching Gaia Science Alerts sources: * SDSS * 2MASS * NED * ASAS * OGLE * INTEGRAL [http://arxiv.org/abs/0910.1704] - Gamma-ray sources, all sky 5eff78a0fa4a2ae077af7746436b73b5aba967ac 274 273 2009-10-12T13:04:02Z Lukasz 2 wikitext text/x-wiki List of catalogues to be used for cross-matching Gaia Science Alerts sources: * SDSS * 2MASS * NED * ASAS [http://www.astrouw.edu.pl/asas/] - long term photometry data in I and V. Whole sky (N+S), down to 14mag * OGLE [http://ogle.astrouw.edu.pl] - long term photometry data in I and V. Bulge and Magellanic Clouds only * INTEGRAL [http://arxiv.org/abs/0910.1704] - Gamma-ray sources, all sky, data available for download [http://integral.esac.esa.int/isda/] 58be792715535eb9322a52c8468ec401af577142 6 87 277 2009-10-12T13:45:18Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 278 277 2009-10-12T13:45:50Z Lukasz 2 uploaded a new version of "[[File:RCRB-nearIR.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 8 280 249 2009-10-23T18:03:35Z Pilecki 15 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:TTau | T Tauri type pre-main sequence stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] ca954e69bb1e1eb5005e93a6302f3020b46ec77c 298 280 2009-11-05T11:46:19Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:TTau | T Tauri type pre-main sequence stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 1f9a1c5881b77fedb0204f9a41b77805aa7acd60 0 88 281 2009-10-23T18:12:09Z Pilecki 15 Created page with '== T Tauri stars == [[File:figure_ttau_mag.png|300px|right|thumb|Example of TTau star from the ASAS data]] Short description. Characteristics: * irregular variations * high amp...' wikitext text/x-wiki == T Tauri stars == [[File:figure_ttau_mag.png|300px|right|thumb|Example of TTau star from the ASAS data]] Short description. Characteristics: * irregular variations * high amplitude * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * ? < V-I < ? 08d0bb80614e26883da72beb510f5c9a9ec6448c 283 281 2009-10-26T02:07:01Z Pilecki 15 wikitext text/x-wiki == T Tauri stars == [[File:figure_ttau_mag.png|400px|right|thumb|Example of TTau star from the ASAS data]] T Tauri type stars are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>) pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. Characteristics: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * ? < V-I < ? 6e145d5edf5fb994ea500e30335bce4da1fff6df 292 283 2009-10-28T19:37:47Z Pilecki 15 wikitext text/x-wiki == T Tauri stars == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>) pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. Characteristics: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * ? < V-I < ? c4ed06f6265597d516fcb1daee7776518abb016f 6 89 282 2009-10-25T22:25:51Z Pilecki 15 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 18 285 46 2009-10-28T15:57:24Z Lukasz 2 /* EX Lupis (EXors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] [[File:ExLupi.gif|right|300pix|thumb|EX Lupi photometry from Herbig(2007).]] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. ade6f6c080ff374309947852bfcd44bb25f94a2a 286 285 2009-10-28T15:58:27Z Lukasz 2 /* EX Lupis (EXors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] [[File:ExLupi.png|right|300pix|thumb|EX Lupi photometry from Herbig(2007).]] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. 0c5055f8bc56815fc71d89317b73c700035cb057 288 286 2009-10-28T15:59:17Z Lukasz 2 /* EX Lupis (EXors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === [[File:ExLupi.png|right|400pix|thumb|EX Lupi photometry from Herbig(2007).]] See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. 58bd02dd9a2e99a23e2170403e6cd23466177bc7 289 288 2009-10-28T15:59:59Z Lukasz 2 /* EX Lupis (EXors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from Herbig(2007).]] See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. 5ee0b914ce38945f51a413a6c02c745f06ac2636 291 289 2009-10-28T16:39:12Z Pilecki 15 wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. 21b0e1ef0e60a8214e5c4b7c064c6a7ab9d51791 6 90 287 2009-10-28T15:58:39Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 290 287 2009-10-28T16:37:46Z Pilecki 15 uploaded a new version of "[[File:ExLupi.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 60 293 166 2009-11-02T18:25:43Z Lukasz 2 wikitext text/x-wiki Links and information on current and future photometric and astrometric surveys: * [http://www.lpl.arizona.edu/css/ Catalina Real-Time Transient Survey], [http://ukads.nottingham.ac.uk/abs/2009ApJ...696..870D Drake et al. 2009] * [http://www.astro.caltech.edu/~george/pq/ Palomar-Quest], [http://ukads.nottingham.ac.uk/abs/2008AN....329..263D Djorgovski et al. 2008] * All Sky Automated Survey ([http://www.astrouw.edu.pl/asas/ ASAS]), [http://ukads.nottingham.ac.uk/abs/2002AcA....52..397P Pojmanski 2002], limited by V~14 mag, all sky survey, observing from Chile since 1997 and from Hawai since 2006. * Optical Gravitational Lensing Experiment ([http://ogle.astrouw.edu.pl OGLE]), [http://adsabs.harvard.edu/abs/2003AcA....53..291U Udalski 2003], Bulge, LMC and SMC only, continuously gathers data since 1996. * SDSS-II Supernova Survey, e.g. Holtzman et al. 2008 * Palomar Transient Factory, e.g. Rau et al. 2009, in operation since Dec.2008 For detailed information on some of the survey please refer to [www.astro.ku.dk/~erik/AstrometricSurveys.pdf Poster by Erik Hog] 797a10379bc2a1cae120a647f63cbdf9e88fc8e7 294 293 2009-11-02T18:26:14Z Lukasz 2 wikitext text/x-wiki Links and information on current and future photometric and astrometric surveys: * [http://www.lpl.arizona.edu/css/ Catalina Real-Time Transient Survey], [http://ukads.nottingham.ac.uk/abs/2009ApJ...696..870D Drake et al. 2009] * [http://www.astro.caltech.edu/~george/pq/ Palomar-Quest], [http://ukads.nottingham.ac.uk/abs/2008AN....329..263D Djorgovski et al. 2008] * All Sky Automated Survey ([http://www.astrouw.edu.pl/asas/ ASAS]), [http://ukads.nottingham.ac.uk/abs/2002AcA....52..397P Pojmanski 2002], limited by V~14 mag, all sky survey, observing from Chile since 1997 and from Hawai since 2006. * Optical Gravitational Lensing Experiment ([http://ogle.astrouw.edu.pl OGLE]), [http://adsabs.harvard.edu/abs/2003AcA....53..291U Udalski 2003], Bulge, LMC and SMC only, continuously gathers data since 1996. * SDSS-II Supernova Survey, e.g. Holtzman et al. 2008 * Palomar Transient Factory, e.g. Rau et al. 2009, in operation since Dec.2008 For detailed information on some of the survey please refer to [www.astro.ku.dk/~erik/AstrometricSurveys.pdf poster] by Erik Hog. c1f521d6f6f78fbad5b8c1ec9d15334b9f0a1ba1 295 294 2009-11-02T18:26:37Z Lukasz 2 wikitext text/x-wiki Links and information on current and future photometric and astrometric surveys: * [http://www.lpl.arizona.edu/css/ Catalina Real-Time Transient Survey], [http://ukads.nottingham.ac.uk/abs/2009ApJ...696..870D Drake et al. 2009] * [http://www.astro.caltech.edu/~george/pq/ Palomar-Quest], [http://ukads.nottingham.ac.uk/abs/2008AN....329..263D Djorgovski et al. 2008] * All Sky Automated Survey ([http://www.astrouw.edu.pl/asas/ ASAS]), [http://ukads.nottingham.ac.uk/abs/2002AcA....52..397P Pojmanski 2002], limited by V~14 mag, all sky survey, observing from Chile since 1997 and from Hawai since 2006. * Optical Gravitational Lensing Experiment ([http://ogle.astrouw.edu.pl OGLE]), [http://adsabs.harvard.edu/abs/2003AcA....53..291U Udalski 2003], Bulge, LMC and SMC only, continuously gathers data since 1996. * SDSS-II Supernova Survey, e.g. Holtzman et al. 2008 * Palomar Transient Factory, e.g. Rau et al. 2009, in operation since Dec.2008 For detailed information on some of the survey please refer to [http://www.astro.ku.dk/~erik/AstrometricSurveys.pdf poster by Erik Hog]. 5eba207273333dbe41a8f4ca6c4d378d342b45f3 296 295 2009-11-02T18:28:30Z Gsawgwikiadmin 1 wikitext text/x-wiki Links and information on current and future photometric and astrometric surveys: * [http://www.lpl.arizona.edu/css/ Catalina Real-Time Transient Survey], [http://ukads.nottingham.ac.uk/abs/2009ApJ...696..870D Drake et al. 2009] * [http://www.astro.caltech.edu/~george/pq/ Palomar-Quest], [http://ukads.nottingham.ac.uk/abs/2008AN....329..263D Djorgovski et al. 2008] * All Sky Automated Survey ([http://www.astrouw.edu.pl/asas/ ASAS]), [http://ukads.nottingham.ac.uk/abs/2002AcA....52..397P Pojmanski 2002], limited by V~14 mag, all sky survey, observing from Chile since 1997 and from Hawai since 2006. * Optical Gravitational Lensing Experiment ([http://ogle.astrouw.edu.pl OGLE]), [http://adsabs.harvard.edu/abs/2003AcA....53..291U Udalski 2003], Bulge, LMC and SMC only, continuously gathers data since 1996. * SDSS-II Supernova Survey, e.g. Holtzman et al. 2008 * Palomar Transient Factory, e.g. Rau et al. 2009, in operation since Dec.2008 For detailed information on some of the survey please refer to [http://www.astro.ku.dk/~erik/AstrometricSurveys.pdf poster by Erik Hoeg]. e92ff0646faf9de9f0a48b7cd893fdf8b0118835 0 80 297 248 2009-11-04T16:05:13Z Lukasz 2 wikitext text/x-wiki Gaia Science Alerts will also provide an opportunity for continuous monitoring of selected objects. Targets can be added or removed anytime during the mission. A tentative list of possible targets include: * R CrB-type stars * FU Ori-type stars * CVs * Novae, recurrent novae * Helium flash stars * Symbiotic stars * Blazars * Gravitationally lensed quasars with resolvable images * Gravitationally lensed galaxies to catch supernovae outbursts c6e43509a3ed241b1ba226da9bb1eae2262e8e99 0 91 299 2009-11-05T12:05:52Z Lukasz 2 Created page with 'Strong lensing of distant galaxies by other galaxies or their clusters can reveal supernovae outbursts in high redshift, otherwise invisible. Gaia will be possible able to detect...' wikitext text/x-wiki Strong lensing of distant galaxies by other galaxies or their clusters can reveal supernovae outbursts in high redshift, otherwise invisible. Gaia will be possible able to detect these as new sources located in vicinity of a gravitational lens. It will probably be limited only to the closest lensed galaxies. [[File:lensedSNexample.png]] from [http://arxiv.org/abs/astro-ph/0007228 Sullivan et al. 2000] 4e9348f2a337da7b7e1e89fb38f3078925502e81 6 92 300 2009-11-05T12:06:15Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 18 301 291 2009-11-05T12:15:35Z Lukasz 2 /* EX Lupis (EXors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) == Similar types to FU Ori == === EX Lupis (EXors) === [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars (see also [[Triggers:TTau]]) === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. cdea3d28bb0e51545e67ffb774db766326896891 302 301 2009-11-05T13:00:55Z Sth 6 /* FU Orionis (FUors) */ wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) References: * The photometric evolution of FU Orionis objects: disc instability and wind-envelope interaction (http://ukads.nottingham.ac.uk/abs/2005MNRAS.361..942C) == Similar types to FU Ori == === EX Lupis (EXors) === [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars (see also [[Triggers:TTau]]) === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. e84b07cd7ba77f3e91496b8123b9e5d4113aefb1 338 302 2009-12-14T15:59:31Z Lukasz 2 wikitext text/x-wiki == FU Orionis (FUors) == FU Orionis (V1647 Ori) is young pre-main sequence stars, illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. Characteristics: * Very rare * Outbursts repeat with a time scale of 40 years (1978, 2003) * Amplitude: 5 mag over 4 months * Outbursts last for 2 years * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * At maximum spectral types are in the range Ae(alpha) - Gpe(alpha) * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) References: * The photometric evolution of FU Orionis objects: disc instability and wind-envelope interaction (http://ukads.nottingham.ac.uk/abs/2005MNRAS.361..942C) == Similar types to FU Ori == === EX Lupis (EXors) === [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] See Herbig (2007) [http://www.iop.org/EJ/article/1538-3881/133/6/2679/205809.text.html] * Recurent eruptions * Amplitudes similar or smaller than in FUors * Balmer emission lines, He I and other lines as in active T Tauri stars (see also [[Triggers:TTau]]) === OO Serpentis === OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. d013693cb38c94a3fddcc372360024b90744d52f 0 10 303 272 2009-11-06T13:18:51Z Lukasz 2 wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] b1097e382011e98dc7080220031a3d7982c7f033 304 303 2009-11-06T13:25:50Z Lukasz 2 wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 7a3ddc590d14ce64dc98384c11a4bcb4a8ec5ce9 307 304 2009-11-06T13:37:20Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 92bcb07e5cec13c42a79c94ec697e70857ea8650 314 307 2009-11-23T15:27:30Z Lukasz 2 wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. A [[Slide-OperationScheme.pdf|slide in PDF]] describing the design of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 7bb41d99336a2faf013282351c72babe09d53f50 315 314 2009-11-23T15:27:49Z Lukasz 2 wikitext text/x-wiki Detailed description (in draft version) of the Java code is available from [http://gaia.esac.esa.int/WebSVN/filedetails.php?repname=DPAC+Subversion+Repository&path=%2FDPAC%2FCU5%2Fdocs%2FGAIA-C5-TN-IOA-LW-002%2FGAIA-C5-TN-IOA-LW-002.pdf Gaia WebSVN] (Gaia password required), or [[Media:fluxalertsmanual.pdf|here]]. A [[Media:Slide-OperationScheme.pdf|slide in PDF]] describing the design of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 558cadefadb48a869145b3b2da3a719099ee0e29 341 315 2009-12-17T16:32:08Z Lukasz 2 wikitext text/x-wiki [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 35c7b7454e5115ac5648e1a7e83dcbb3f47615c7 6 93 305 2009-11-06T13:26:07Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 306 305 2009-11-06T13:28:59Z Lukasz 2 uploaded a new version of "[[File:Scanning law gal.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 1 308 37 2009-11-11T08:55:53Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 323bb771de0695a2972717414749182292156797 6 53 309 126 2009-11-16T12:35:56Z Lukasz 2 uploaded a new version of "[[File:Plot transients tau ampl.png]]": GRBs added wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 55 310 128 2009-11-16T12:38:44Z Lukasz 2 uploaded a new version of "[[File:Plot transients trise ampl.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 54 311 127 2009-11-16T12:39:37Z Lukasz 2 uploaded a new version of "[[File:Plot transients tdecline ampl.png]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 24 312 80 2009-11-17T12:05:52Z Lukasz 2 /* OGLE and MACHO data were studied for Be stars. */ wikitext text/x-wiki == OGLE and MACHO data were studied for Be stars.== * OGLE (LMC,SMC): [http://ukads.nottingham.ac.uk/abs/2005MNRAS.361.1055S Sabogal et al. 2005], [http://ukads.nottingham.ac.uk/abs/2006A%26A...457..949M Mennickent et al. 2006] * OGLE (Bulge): [http://ukads.nottingham.ac.uk/abs/2008A%26A...478..659S Sabogal et al. 2008] 29,000 found in OGLE-II Bulge fields. * MACHO: [http://ukads.nottingham.ac.uk/abs/2002AJ....124.2039K Keller et al. 2002] 1279 found in MACHO LMC data. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] 2b7418418294c86820f888273c2149f3b11641d0 6 94 313 2009-11-23T15:25:32Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 40 316 246 2009-11-26T10:37:25Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Thumb|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Thumb|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] c585de1f23b27a47e9cebd1ea322a29507ff34c0 319 316 2009-11-26T10:38:35Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|400px|thumb|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|400px|thumb|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] c83b1f87223b558a85ca4a365ac9242982e42b35 320 319 2009-11-26T10:39:01Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == [[File:SN2008iy-phot.png|400px|thumb|left|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|400px|thumb|right|Spectrometry of SN2008iy. d is the time of discovery.]] Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] c1103138950427bb537191b6941a4003a52bbfbf 321 320 2009-11-26T10:39:15Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == [[File:SN2008iy-phot.png|300px|thumb|left|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|thumb|right|Spectrometry of SN2008iy. d is the time of discovery.]] Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] 192654a44506aac804102de606d54dadd7b2d80a 322 321 2009-11-26T10:40:01Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] 866316f4c2431c78965f30b55e8e37740b154fdb 323 322 2009-11-26T10:40:17Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans (1993: MNRAS, 341, 569-576). Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokuroav and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] 1466924ccd45e596c03f3efa578eeab67e3bbb49 346 323 2010-02-11T10:53:12Z Lukasz 2 wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] a34bd4c67454c54a3b0a0e9d7902f28b1a6743af 347 346 2010-02-11T10:59:19Z Lukasz 2 /* Supernovae type Ia */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days'''. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] f0300de92e849b73cb781b046562b678f3abf162 348 347 2010-02-11T11:01:51Z Lukasz 2 /* Rise and fall times of SN Ia */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] 6da929723d22dce7a1e56ea19239d8cb410fc7d6 6 95 317 2009-11-26T10:37:46Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 96 318 2009-11-26T10:38:04Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 17 324 140 2009-11-26T14:20:14Z Lukasz 2 /* Current and future instruments suitable for Gaia alerts response */ wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == '''Please list here any surveys probable to be in operation from 2012 to 2017 suitable for following-up Gaia alerts.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 74fd06d695f9472ce2b36aa985eda55551962ebb 0 15 325 175 2009-12-01T13:33:25Z Lukasz 2 wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of massive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star * no radio or X-ray counterpart detected * no star visible at that location prior to the outburst on HST archival images. [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. ---- == OT060420 == Very short (~12 min) and bright (~ 5 mag) transient detected by CONCAM all-sky cameras [http://arxiv.org/abs/astro-ph/0607033]. The astronomical nature of the event is disputable, as the detection was made only on two out of three telescopes. One explanation is that the transient was variable. Gaia will be able to detect such transients and also provide per-ccd photometry, every 4 seconds. ---- == Optical transients due to unbound tidal debris == See [http://uk.arxiv.org/abs/0911.5358 Kasen & Ramirez-Ruiz 2009] 942ed8c31432cbf28f99533e86d5aabc2f3f764f 344 325 2010-01-19T16:08:37Z Lukasz 2 wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of massive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star * no radio or X-ray counterpart detected * no star visible at that location prior to the outburst on HST archival images. [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. ---- == OT060420 == Very short (~12 min) and bright (~ 5 mag) transient detected by CONCAM all-sky cameras [http://arxiv.org/abs/astro-ph/0607033]. The astronomical nature of the event is disputable, as the detection was made only on two out of three telescopes. One explanation is that the transient was variable. Gaia will be able to detect such transients and also provide per-ccd photometry, every 4 seconds. ---- == Optical transients due to unbound tidal debris == See [http://uk.arxiv.org/abs/0911.5358 Kasen & Ramirez-Ruiz 2009] ---- == Quasar flares (?) == See [http://uk.arxiv.org/abs/1001.2991 Meusinger et al. 2010] 5ced92133b47cdaa5af6011d8fd26461520c8780 6 97 326 2009-12-08T08:58:34Z Vojtechsimon 11 Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs. The color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble wikitext text/x-wiki Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs. The color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble (Simon et al. 2001, 2004} are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown. Adapted from Simon et al. (2001, 2004), where a detailed information can be found. 272dc4793db3ee859ced4d209cad068789c6ee04 0 73 327 262 2009-12-08T09:44:26Z Vojtechsimon 11 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs. The color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble (Simon , Sim04} are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown. Adapted from Simon et al. (2001, 2004), where a detailed information can be found. 7133941fa2b5e3f15c201f2447fbb8149a930232 328 327 2009-12-08T09:56:01Z Vojtechsimon 11 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Very short-lived optical transients associated with enormous gamma-ray outbursts. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * time-scales from seconds to minutes * in maximum can reach up to few mag, but the whole range observed * host galaxy can be visible [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. The color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown. Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 18a113146603c7c9d94aa095b4365bda3b03ea74 330 328 2009-12-08T10:27:00Z Vojtechsimon 11 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Short-lived optical transients associated with enormous gamma-ray outbursts GRBs. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * Time-scales of the gamma-ray emission range from a fraction of second to several minutes. This emission is often accompanied by the so-called optical afterglow which can last for several days. * Optical afterglow can reach up to few mag in maximum, but the whole range of magnitudes observed at a given time elapsed from the GRB largely differs for the individual events (more than 3 mag). These optical afterglows often display specific color indices with negligible time evolution, which helps distinguish them from other kinds of transients. * Host galaxy of GRB can be visible, but its apprent magnitude is usually fainter than the detection limit of Gaia (about 20 mag). Nevertheless, this host galaxy can often be detected by large ground-based telescopes at the position of the optical afterglow. [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. The color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown. Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 6927513acc416807725c25c9937147b812b1a659 337 330 2009-12-09T11:46:34Z Vojtechsimon 11 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Short-lived optical transients associated with enormous gamma-ray outbursts GRBs. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * Time-scales of the gamma-ray emission range from a fraction of second to several minutes. This emission is often accompanied by the so-called optical afterglow which can last for several days. Optical afterglows can be therefore detected with Gaia even several days after the GRB trigger. * Optical afterglow can reach up to few mag in maximum, but the whole range of magnitudes observed at a given time elapsed from the GRB largely differs for the individual events (more than 3 mag). These optical afterglows often display specific color indices with negligible time evolution, which helps distinguish them from other kinds of transients by photometric observations using several color filters. * Host galaxy of GRB can be visible, but its apprent magnitude is usually fainter than the detection limit of Gaia (about 20 mag). Nevertheless, this host galaxy can often be detected by large ground-based telescopes at the position of the optical afterglow. [[File:GRB06-RAPTOR.png|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. dea4aa8982a7707473eeefd166ac08b77559b9be 0 7 329 13 2009-12-08T09:59:26Z Vojtechsimon 11 wikitext text/x-wiki ==People contributing to the Science Alerts Working Group== ''Add your name here if you contribute.'' * Institute of Astronomy, Cambridge, UK ** [[user:Lukasz|Lukasz Wyrzykowski]] ** [[user:STH | Simon Hodgkin]] ** [[user:Vasily | Vasily Belokurov]] * Astronomical Institute, AS CR, Czech Republic ** [[Vojtech Simon]] 0e1fb3f9a6c94aabd5a3a7ec4e015606bd2e2bdc 0 8 331 298 2009-12-08T10:31:46Z Vojtechsimon 11 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Supernovae | Supernovae]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:XBs | X-ray binaries (XBs)]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:TTau | T Tauri type pre-main sequence stars]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 68ab274dd3fbe2a04fdcc1ce816c96f6ce3c35c2 6 98 332 2009-12-08T12:57:59Z Vojtechsimon 11 Types of CVs according to the increasing mass transfer rate wikitext text/x-wiki Types of CVs according to the increasing mass transfer rate 99f83123aa8d087e7bed759027b74366569bc126 0 81 333 257 2009-12-08T13:00:44Z Vojtechsimon 11 wikitext text/x-wiki There is a very large variety of behaviours of CVs. [[File:Types-of-CVs.png|400px|]] == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. * V504 Cen has period of 4.21h and went down by 6 mag in 2006 and remained in it for nearly a year. c8d6bdb6fb51384403f8632c2e331b8d3863f2b4 334 333 2009-12-08T14:15:00Z Vojtechsimon 11 wikitext text/x-wiki Cataclysmic variables (CVs) are very active objects and their long-term activity is extremely complex. No two CVs display identical activity. The current state of art explains this variety as a result of two dominant physical processes – variations of the mass transfer rate d''m''/d''t'' with time (i.e. changes of the amount of matter which is being transferred from the companion star (donor) to the WD), and the thermal instability of the accretion disk. It emerges that the complicated profiles of the light curves basicly result from a combination of these two mechanisms (e.g. [http://adsabs.harvard.edu/abs/1995CAS....28.....W Warner, 1995]). The basic systematics of the long-term activity in CVs, shown in Fig.2, can be arranged in the following way: [[File:Types-of-CVs.png|400px|]] == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. * V504 Cen has period of 4.21h and went down by 6 mag in 2006 and remained in it for nearly a year. 3231c7442d2d49b66b32bd8731faa9e4688816f9 335 334 2009-12-08T14:34:29Z Vojtechsimon 11 wikitext text/x-wiki Cataclysmic variables (CVs) are very active objects and their long-term activity is extremely complex. No two CVs display identical activity. The current state of art explains this variety as a result of two dominant physical processes – variations of the mass transfer rate d''m''/d''t'' with time (i.e. changes of the amount of matter which is being transferred from the companion star (donor) to the WD), and the thermal instability of the accretion disk. It emerges that the complicated profiles of the light curves basicly result from a combination of these two mechanisms (e.g. [http://adsabs.harvard.edu/abs/1995CAS....28.....W Warner, 1995]). The basic systematics of the long-term activity in CVs, can be arranged in the following way, as shown in the following three panels. From top to bottom panel, the character of this activity changes from large-amplitude, isolated outbursts starting from the low baseline brightness to the dominant relatively small fluctuations in the high state. [[File:Types-of-CVs.png|400px|]] == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. * V504 Cen has period of 4.21h and went down by 6 mag in 2006 and remained in it for nearly a year. b4e7d8f7b25a7471ff947cdddb59e7f3f9c3d1cf 336 335 2009-12-08T14:58:54Z Vojtechsimon 11 wikitext text/x-wiki Cataclysmic variables (CVs) are very active objects and their long-term activity is extremely complex. No two CVs display identical activity. The current state of art explains this variety as a result of two dominant physical processes – variations of the mass transfer rate d''m''/d''t'' with time (i.e. changes of the amount of matter which is being transferred from the companion star (donor) to the WD), and the thermal instability of the accretion disk. It emerges that the complicated profiles of the light curves basicly result from a combination of these two mechanisms (e.g. [http://adsabs.harvard.edu/abs/1995CAS....28.....W Warner, 1995]). The basic systematics of the long-term activity in CVs, can be arranged in the following way, as shown in the following three panels. From top to bottom panel, the character of this activity changes from large-amplitude, isolated outbursts starting from the low baseline brightness to the dominant relatively small fluctuations in the high state. [[File:Types-of-CVs.png|400px|]] == Basic properties of the long-term activity in various kinds of CVs == The basic observable parameters of the long-term brightness variations can be summarized in the following way. Time-averaged d''m''/d''t'' increases in the sequence: ''Dwarf novae of U Gem type'' ''Dwarf novae of Z Cam type'' ''Novalike'' (Dwarf novae of SU UMa type are CVs with very short orbital period (mostly less than 2 hours). Their activity is similar to U Gem type, but they display two types of outburst - normal outbursts and superoutbursts.) * '''Dwarf novae of U Gem type – rare outbursts''' **Typical duration of outburst: days to weeks **Typical recurrence time (cycle-length) of outbursts: weeks to years **Typical amplitude of outburst: 2-7 mag *'''Dwarf novae of SU UMa type''' **Typical duration of a normal outburst: days **Typical recurrence time (cycle-length) of normal outbursts: weeks to years **Typical amplitude of a normal outburst: 2-3 mag **Typical duration of a superoutburst: two weeks **Typical recurrence time (cycle-length) of superoutbursts: weeks to years **Typical amplitude of a superoutburst: 3-5 mag *'''Dwarf novae of Z Cam type''' **Typical duration of outburst: days to 1 week **Typical recurrence time (cycle-length) of outbursts: weeks **Typical amplitude of outburst: 2-3 mag *'''Novalike and VY Scl type systems''' **Typical timescale of fluctuations: days to weeks **Typical amplitude of fluctuations: 0.5-1 mag **Typical amplitude of high/low state transitions: 1-4 mag == VY Sculptoris == A subclass of cataclysmic variables exhibiting occasional drops by several magnitudes at irregular intervals. The prototype of the class had shown a deep low-state in 2008, first since 1983 ([http://uk.arxiv.org/abs/0910.0475 Greiner et al. 2009]). [[File:CV-VYScl.png|300px|right]] * amplitude: several magnitudes * drop time scale: 10-30 days * low state lasts for about 100 days * some periodicity (P about 10 days) is present * mechanism not well understood * some of VY Scl stars are supersoft X-ray sources during optical low-states. * V504 Cen has period of 4.21h and went down by 6 mag in 2006 and remained in it for nearly a year. 3a42e49c0d2343198454780d26b5ba7756b9ce05 0 50 339 119 2009-12-14T16:05:47Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra of novae near maximum light resemble A-F absorption spectra of luminous stars at first * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days 9dc5111c2fc32951988e80e14a7ce900b2b0af9b 340 339 2009-12-14T16:07:05Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra near maximum light resemble A-F absorption spectra of luminous stars at first * spectra at minimum light resemble spectra of Wolf-Rayet stars. * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days 8db9c97998c2250ba39f8a954776d985d27b6017 6 99 342 2009-12-17T16:32:45Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 20 343 120 2010-01-05T12:41:28Z Lukasz 2 wikitext text/x-wiki DNe are cataclysmic variable stars consisting of a close binary star system in which one of the components is a white dwarf, which accretes matter from its companion. They are similar to classical novae in that the white dwarf is involved in periodic outbursts, but the mechanisms are different: classical novae result from the fusion and detonation of accreted hydrogen, while current theory suggests that dwarf novae result from instability in the accretion disk, when gas in the disk reaches a critical temperature that causes a change in viscosity, resulting in a collapse onto the white dwarf that releases large amounts of gravitational potential energy[http://en.wikipedia.org/wiki/Dwarf_nova]. * They repeat on irregular intervals of a few weeks to years. * Amplitude up to 6 mag, with <math>A=0.8+1.667 \log(\Delta t_{repeat})</math> * typical DN have two different types of outbursts: more and less energetic. * Classes: U Gem, Z Cam, SU UMa * in the baseline can show small variation with periods in range 0.05-0.5 days. * often accompanied by X-ray emission * spectrum of a system at minimum is continuous, with broad H and He emission lines * spectrum at maximum: the lines almost disappear or become shallow absorption lines[http://www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/vartype.txt] Example of a dwarf nova GK Perseii ([http://arxiv.org/abs/0907.1407 Evans et al. 2009]) : detection of an outburst led to Swift, UV and X-rays follow up. It revealed unusual outburst in the optical but typical outburst in X, challenging existing disc outburst models. [[File:GKPer.png|400px|thumb|left|AAVSO lightcurve of outbursts of dwarf nova GK Per since 1954]] 5fe0ad315a0fddd42b38177e1d4dad0280d09a50 0 91 345 299 2010-02-09T12:58:05Z Lukasz 2 wikitext text/x-wiki Strong lensing of distant galaxies by other galaxies or their clusters can reveal supernovae outbursts in high redshift, otherwise invisible. Gaia will be possible able to detect these as new sources located in vicinity of a gravitational lens. It will probably be limited only to the closest lensed galaxies. [[File:lensedSNexample.png]] from [http://arxiv.org/abs/astro-ph/0007228 Sullivan et al. 2000] Example application of lensed SNe: modelling the dark matter haloes of lensing galaxies ([http://uk.arxiv.org/abs/1002.1374 Jonsson et al. 2010]. 9478d1fbfc4f6b969d46c117966995d502933573 8 3 349 247 2010-02-25T16:36:31Z Gsawgwikiadmin 1 wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2010 ** main|Main Workshop Page ** rationale|Rationale ** agenda|Agenda ** registration|Registration ** logistics|Logistics * SEARCH * TOOLBOX 6c528bd247d967aef13159c6de971200d9fda688 350 349 2010-02-25T16:37:29Z Gsawgwikiadmin 1 wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2010 ** workshop2010:main|Main Workshop Page ** workshop2010:rationale|Rationale ** workshop2010:agenda|Agenda ** workshop2010:registration|Registration ** workshop2010:logistics|Logistics * SEARCH * TOOLBOX a90db94280ef7fe1b8b19ae3017c49308c91968e 0 1 351 308 2010-02-25T16:50:40Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- [[Workshop2010:main|Gaia Science Alerts Workshop 2010]]. ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 25407b6c0409fc3642aa10a17c68b84c8e53bc7b 370 351 2010-02-25T18:13:20Z Gsawgwikiadmin 1 /* Welcome to the web site of the Gaia Science Alerts Working Group! */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>'''[[Workshop2010:main|Gaia Science Alerts Workshop 2010]]'''</Big></center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 23ee29d719575d45ed26b01c589ec1f1a0337dd6 0 100 352 2010-02-25T16:53:12Z Gsawgwikiadmin 1 Created page with '== Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010.' wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. 3ee1e2e403a8e307df6b8a20c1675d2cd665304f 368 352 2010-02-25T18:10:09Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] 55e5aaf8c5dea46c9feac865e2a23b5e7348081b 371 368 2010-02-25T18:16:35Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''14 May 2010''' * Invitations allocated: '''14 May 2010''' 051a6e68d4034c5abd0d71948621910588174524 8 101 353 2010-02-25T16:59:17Z Gsawgwikiadmin 1 Created page with '/* CSS placed here will be applied to all skins */ .firstHeading { display:none !important; }' css text/css /* CSS placed here will be applied to all skins */ .firstHeading { display:none !important; } 7ddde6bc1f4a4ba30c75184569c99ea3bbcd9db4 0 102 354 2010-02-25T17:16:49Z Gsawgwikiadmin 1 Created page with 'Gaia will repeatedly monitor the whole sky in the optical. The Gaia Science Alerts stream therefore represents a unique opportunity, and holds a significant responsibility. Trig...' wikitext text/x-wiki Gaia will repeatedly monitor the whole sky in the optical. The Gaia Science Alerts stream therefore represents a unique opportunity, and holds a significant responsibility. Triggers from transient phenomena are the first data that the astronomical community will see from the satellite. It is up the Gaia Science Alerts Team to make sure that the alert stream is accurate, reliable, interesting and free from (or at least acceptably low in) contamination. It is vital to make sure that the astronomical community is ready for these Gaia alerts, and that Gaia starts delivering science quickly. In addition, we will raise public awareness about (and involvement with) the satellite very early on in the mission. == The motivation for the workshop: == * To focus community attention on the scientific possibilities that will arise from the Gaia Science Alerts data stream, and to make sure that astronomers are prepared and motivated to exploit the data as it arrives. * To invite the community to influence the scope of the science alerts processing algorithms and alert strategies, to ensure that returns from the mission are maximized, and that exciting opportunities are not overlooked. == Target participants: == # Experts on the Gaia mission and data flow system, together with developers and scientists working on the Science Alerts System. # Astronomers who are actively involved or interested in ongoing or planned surveys for transient phenomena, for example the Palomar Transient Factory, the Catalina Survey, the Supernova Factory, PanSTARRS, LSST, WASP, OGLE, ASAS. # Active researchers into transient phenomena, such as Supernovae, Microlensing Events, Gamma Ray Bursts, Classical Novae, ExtraGalactic variability, CVs, Be stars, massive stars and so on. # Scientists who are involved in the distribution of Alert information, e.g. from eSTAR and GCN # Individuals who are interested in the outreach possibilities of Gaia Science Alerts. 0853cbd60dc4786d84ff9d9ee992bf72e1909e04 355 354 2010-02-25T17:17:16Z Gsawgwikiadmin 1 wikitext text/x-wiki = Workshop's Rationale == Gaia will repeatedly monitor the whole sky in the optical. The Gaia Science Alerts stream therefore represents a unique opportunity, and holds a significant responsibility. Triggers from transient phenomena are the first data that the astronomical community will see from the satellite. It is up the Gaia Science Alerts Team to make sure that the alert stream is accurate, reliable, interesting and free from (or at least acceptably low in) contamination. It is vital to make sure that the astronomical community is ready for these Gaia alerts, and that Gaia starts delivering science quickly. In addition, we will raise public awareness about (and involvement with) the satellite very early on in the mission. == The motivation for the workshop: == * To focus community attention on the scientific possibilities that will arise from the Gaia Science Alerts data stream, and to make sure that astronomers are prepared and motivated to exploit the data as it arrives. * To invite the community to influence the scope of the science alerts processing algorithms and alert strategies, to ensure that returns from the mission are maximized, and that exciting opportunities are not overlooked. == Target participants: == # Experts on the Gaia mission and data flow system, together with developers and scientists working on the Science Alerts System. # Astronomers who are actively involved or interested in ongoing or planned surveys for transient phenomena, for example the Palomar Transient Factory, the Catalina Survey, the Supernova Factory, PanSTARRS, LSST, WASP, OGLE, ASAS. # Active researchers into transient phenomena, such as Supernovae, Microlensing Events, Gamma Ray Bursts, Classical Novae, ExtraGalactic variability, CVs, Be stars, massive stars and so on. # Scientists who are involved in the distribution of Alert information, e.g. from eSTAR and GCN # Individuals who are interested in the outreach possibilities of Gaia Science Alerts. 17d74d5398ef4fbeadb773c0be96eb6fc43472b0 356 355 2010-02-25T17:17:25Z Gsawgwikiadmin 1 wikitext text/x-wiki = Workshop's Rationale = Gaia will repeatedly monitor the whole sky in the optical. The Gaia Science Alerts stream therefore represents a unique opportunity, and holds a significant responsibility. Triggers from transient phenomena are the first data that the astronomical community will see from the satellite. It is up the Gaia Science Alerts Team to make sure that the alert stream is accurate, reliable, interesting and free from (or at least acceptably low in) contamination. It is vital to make sure that the astronomical community is ready for these Gaia alerts, and that Gaia starts delivering science quickly. In addition, we will raise public awareness about (and involvement with) the satellite very early on in the mission. == The motivation for the workshop: == * To focus community attention on the scientific possibilities that will arise from the Gaia Science Alerts data stream, and to make sure that astronomers are prepared and motivated to exploit the data as it arrives. * To invite the community to influence the scope of the science alerts processing algorithms and alert strategies, to ensure that returns from the mission are maximized, and that exciting opportunities are not overlooked. == Target participants: == # Experts on the Gaia mission and data flow system, together with developers and scientists working on the Science Alerts System. # Astronomers who are actively involved or interested in ongoing or planned surveys for transient phenomena, for example the Palomar Transient Factory, the Catalina Survey, the Supernova Factory, PanSTARRS, LSST, WASP, OGLE, ASAS. # Active researchers into transient phenomena, such as Supernovae, Microlensing Events, Gamma Ray Bursts, Classical Novae, ExtraGalactic variability, CVs, Be stars, massive stars and so on. # Scientists who are involved in the distribution of Alert information, e.g. from eSTAR and GCN # Individuals who are interested in the outreach possibilities of Gaia Science Alerts. 972373a004780ffbaa09ad7de3503572a8637ed9 0 103 357 2010-02-25T17:20:33Z Gsawgwikiadmin 1 Created page with '=Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not...' wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. Please register HERE to apply for an invitation. ''If you already received an invitation you can relax and start planning you journey to Cambridge!'' ---- Please note, there is no registration fee and the coffee/tea and lunches are free thanks to generous support of ESF grant [[GREAT|http://www.ast.cam.ac.uk/GREAT/]] [[File:great-esf-logo.png]] GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until 30 April 2010. Please specify your needs in the application form above. d3d148ad819cc4aa1a28ccb10f56b2fce0af8ca3 358 357 2010-02-25T17:21:40Z Gsawgwikiadmin 1 /* Registration */ wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. Please register HERE to apply for an invitation. ''If you already received an invitation you can relax and start planning you journey to Cambridge!'' ---- Please note, there is no registration fee and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. [[File:great-esf-logo.png]] GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until 30 April 2010. Please specify your needs in the application form above. 1c72a88a1df53def3c1fd53682728e86c44f77f9 360 358 2010-02-25T17:23:24Z Gsawgwikiadmin 1 /* Registration */ wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. Please register HERE to apply for an invitation. ''If you already received an invitation you can relax and start planning you journey to Cambridge!'' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until 30 April 2010. Please specify your needs in the application form above. d987998dcfec9684a606a650198a2daa8402bce5 361 360 2010-02-25T17:25:37Z Gsawgwikiadmin 1 /* Registration */ wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. Please register HERE to apply for an invitation. ''If you already received an invitation you can relax and start planning you journey to Cambridge!'' ---- [[File:great-esf-logo.png|right|200px]] ==== Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. ==== GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until 30 April 2010. Please specify your needs in the application form above. 0030ae4e85183b9abbbafd72833a966c551a181b 362 361 2010-02-25T17:28:19Z Gsawgwikiadmin 1 wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Please register HERE to apply for an invitation.</big> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] <big> Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. </big> GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. a2e678a97c708eee2124c7109dd8cdfbd54b78a4 373 362 2010-02-26T10:53:45Z Lukasz 2 /* Registration */ wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Please register HERE to apply for an invitation.</big> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. e3e559d1fc1bd27eb5b6878dc6a034fa04855a1a 374 373 2010-02-26T12:41:38Z Lukasz 2 wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Please register [[workshop2010:registrationform | HERE]] to apply for an invitation.</big> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 17321f2071bbc821025141c6b04e6d976a7c0020 6 104 359 2010-02-25T17:22:08Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 105 363 2010-02-25T18:00:36Z Gsawgwikiadmin 1 Created page with '=Logistics= == Workshop venue == The workshop will take place in the [http://www.ast.cam.ac.uk Institute of Astronomy] at the University of Cambridge. == Accommodation == The...' wikitext text/x-wiki =Logistics= == Workshop venue == The workshop will take place in the [http://www.ast.cam.ac.uk Institute of Astronomy] at the University of Cambridge. == Accommodation == The organizers have booked number of rooms in the nearby Churchill College. Please contact ????? if you are interested in taking this accommodation. Number of rooms is limited. Alternatively, several websites provide a extensive list of hotels and B&B in the Cambridge area. Please check out one of the following: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the Institute of Astronomy but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 5cffecd984e509fc3801c15e0feeaedc49a0a18d 364 363 2010-02-25T18:01:26Z Gsawgwikiadmin 1 wikitext text/x-wiki =Logistics= == Workshop venue == The workshop will take place in the [http://www.ast.cam.ac.uk Institute of Astronomy] at the University of Cambridge. == Accommodation == The organizers have booked number of rooms in the nearby Churchill College. Please contact ????? if you are interested in taking this accommodation. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the Institute of Astronomy but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. fe085f5d1fd5ca052e76d2103265e574a284c534 365 364 2010-02-25T18:04:16Z Gsawgwikiadmin 1 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby Churchill College. Please contact ????? if you are interested in taking this accommodation. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 1efe739b29a594394c285a9cfef002a3824f780d 366 365 2010-02-25T18:07:01Z Gsawgwikiadmin 1 /* Getting to the Institute of Astronomy */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby Churchill College. Please contact ????? if you are interested in taking this accommodation. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 2591f14c7c28cbc3cc825921c8495e71c0592187 367 366 2010-02-25T18:07:53Z Gsawgwikiadmin 1 /* Getting to the Institute of Astronomy */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby Churchill College. Please contact ????? if you are interested in taking this accommodation. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 09df3834bee54f276f2cbf6a481e486b2aa92dc5 372 367 2010-02-25T19:29:08Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. Please contact ????? if you are interested in taking this accommodation. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 9ca2a8d5e65d0b178566b47569add9c29386aed5 0 106 369 2010-02-25T18:11:50Z Gsawgwikiadmin 1 Created page with '=Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00 * Friday 25 June - workshop ends with lunch at 13:00' wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00 * Friday 25 June - workshop ends with lunch at 13:00 c8f6d5a0928f6b3be65494d76c4f480c0e571b52 0 107 375 2010-02-26T12:43:05Z Lukasz 2 Created page with '<form name="test" method="email" target="wyrzykow@gmail.com" email="Registration Test" sender="gsaw2010registration@ast.cam.ac.uk" submit="Send Inquiry" reset="Reset"> hidden...' wikitext text/x-wiki <form name="test" method="email" target="wyrzykow@gmail.com" email="Registration Test" sender="gsaw2010registration@ast.cam.ac.uk" submit="Send Inquiry" reset="Reset"> hidden: name="testform" value="additional info" text:* name="name" prompt="Your [[RealName]]" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text:* name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 6ed1b0b0ce3a95ae7ba989534f5f4b11918233d0 376 375 2010-02-26T12:46:48Z Lukasz 2 wikitext text/x-wiki <form name="test" method="email" target="wyrzykow@gmail.com" email="wyrzykow@ast.cam.ac.uk" submit="Send Inquiry" reset="Reset"> hidden: name="testform" value="additional info" text:* name="name" prompt="Your [[RealName]]" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text:* name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 4229aa8e7fb3f75b2c723e2abe08850c14d924aa 377 376 2010-02-26T12:48:42Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="test" method="email" target="wyrzykow@gmail.com" email="wyrzykow@ast.cam.ac.uk" submit="Send Inquiry" reset="Reset"> hidden: name="testform" value="additional info" text:* name="name" prompt="Your [[RealName]]" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text:* name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 0347ffe2f9a91b16a4d882f1376188818230b305 378 377 2010-02-26T12:49:03Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="test" method="email" target="wyrzykow@gmail.com" email="email" submit="Send Inquiry" reset="Reset"> hidden: name="testform" value="additional info" text:* name="name" prompt="Your [[RealName]]" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text:* name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 77480eba2bc5006381c122d12a7d0dfb7a15adc9 379 378 2010-02-26T12:50:43Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" target="wyrzykow@gmail.com" email="email" submit="Send the form" reset="Reset"> hidden: name="testform" value="additional info" text: name="name" prompt="Your [[RealName]]" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> bd791bba28e6d2247ca739211f2d077a8fbc5e2b 380 379 2010-02-26T12:51:05Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" target="wyrzykow@gmail.com" email="email" submit="Send the form" reset="Reset"> hidden: name="testform" value="additional info" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 488e672fdc9265250d3cdd56457c1e834622b94a 381 380 2010-02-26T12:54:00Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" target="wyrzykow@gmail.com" email="email" submit="Send the form" reset="Reset"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 977341fe5a73b83d12eb88ba4c06105f72f403bc 382 381 2010-02-26T12:54:27Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" target="wyrzykow@gmail.com" submit="Send the form" reset="Reset"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 5b232ce8217f9326a5f996eaa5901a6f7af96118 383 382 2010-02-26T13:03:37Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" submit="Send the form" reset="Reset"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 71853c918cc6ed02b077fdd2eb0a3e73653c8362 384 383 2010-02-26T13:03:56Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" submit="Send the form" reset="clear"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 87df70b991b04d05d6da32f518b5b1d2657ea7f5 385 384 2010-02-26T13:04:21Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear" submit="send"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 5f0a647d944b698689db9d2b278be02f8b054125 386 385 2010-02-26T13:04:34Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear" submit="push"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 7d56b5b2582a8a863e0c0f18882b866dd0ff7f17 387 386 2010-02-26T13:11:55Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear the form" submit="send"> hidden: name="testform" value="additional info" text: name="email" prompt="Your email" text: name="name" prompt="Your Name" select: name="category" prompt="Please select problem category" option="Linux Software" option="Linux Hardware" text: name="summary" prompt="Problem summary" textarea: name="description" prompt="Problem description" rows="10" cols="50" select: name="priority" prompt="Priority" option="Low" option="Medium" option="High" value="Medium" </form> 7071dc8bdfc44ba2e1f9d9ce60961b5dc131c70f 388 387 2010-02-26T13:22:39Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear the form" submit="send"> hidden: name="testform" value="additional info" text: name="name" prompt="Name with title" text: name="affiliation" prompt="Affiliation" textarea: name="address" prompt=Address" rows="4" cols="50" text: name="email" prompt="Email" text: name="tel" prompt="Telephone" Contribution: select: name="contribution" prompt="Please select" option="none" option="talk" option="poster" value="none" text: name="title" prompt="Title" textarea: name="abstract" prompt="Abstract" rows="10" cols="50" Application for funding: select: name="funding" prompt="I would like to apply for funding" option="No" option="Yes" value="No" text: name="funding_amount" prompt="Requested support (in euros)" </form> 58b7382ad13da0cbca6707d2927ddfbf513f7be1 389 388 2010-02-26T13:24:23Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear the form" submit="send"> hidden: name="testform" value="additional info" text: name="name" prompt="Name with title" text: name="affiliation" prompt="Affiliation" textarea: name="address" prompt=Address" rows="4" cols="50" text: name="email" prompt="Email" text: name="tel" prompt="Telephone" select: name="contribution" prompt="Contribution to the workshop" option="none" option="talk" option="poster" value="none" text: name="title" prompt="Title" textarea: name="abstract" prompt="Abstract" rows="10" cols="50" select: name="funding" prompt="I would like to apply for funding" option="No" option="Yes" value="No" text: name="funding_amount" prompt="Requested support (in euros)" </form> c96bf7322c544bed4ede2d7aaf217fd53431fc97 390 389 2010-02-26T13:25:51Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear the form" submit="send"> hidden: name="testform" value="additional info" text: name="name" prompt="Name" text: name="position" prompt="Position" text: name="affiliation" prompt="Affiliation" textarea: name="address" prompt=Address" rows="4" cols="50" text: name="email" prompt="Email" text: name="tel" prompt="Telephone" select: name="contribution" prompt="Contribution to the workshop" option="none" option="talk" option="poster" value="none" text: name="title" prompt="Title" textarea: name="abstract" prompt="Abstract" rows="10" cols="50" select: name="funding" prompt="I would like to apply for funding" option="No" option="Yes" value="No" text: name="funding_amount" prompt="Requested support (in euros)" </form> e812a20fad17da3d97a625441debabdd60bf1be1 391 390 2010-02-26T13:29:52Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="wyrzykow@gmail.com" target="wyrzykow@gmail.com" reset="clear the form" submit="send"> text: name="name" prompt="Name" text: name="position" prompt="Position" text: name="affiliation" prompt="Affiliation" textarea: name="address" prompt="Address" rows="4" cols="50" text: name="email" prompt="Email" text: name="tel" prompt="Telephone" select: name="contribution" prompt="Contribution to the workshop" option="none" option="talk" option="poster" value="none" text: name="title" prompt="Title" textarea: name="abstract" prompt="Abstract" rows="10" cols="50" select: name="funding" prompt="I would like to apply for funding" option="No" option="Yes" value="No" text: name="funding_amount" prompt="Requested support (in euros)" </form> 567015ffa4eeea820e5155f921aeca3f519d176a 392 391 2010-02-26T13:41:51Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- <form name="reg" method="email" email="Your email" target="wyrzykow@gmail.com" reset="clear the form" submit="send"> text: name="name" prompt="Name" text: name="position" prompt="Position" text: name="affiliation" prompt="Affiliation" textarea: name="address" prompt="Address" rows="4" cols="50" text: name="email" prompt="Email" text: name="tel" prompt="Telephone" select: name="contribution" prompt="Contribution to the workshop" option="none" option="talk" option="poster" value="none" text: name="title" prompt="Title" textarea: name="abstract" prompt="Abstract" rows="10" cols="50" select: name="funding" prompt="I would like to apply for funding" option="No" option="Yes" value="No" text: name="funding_amount" prompt="Requested support (in euros)" </form> fc0883605e3d0683be95b73d445162ad08443f1c 394 392 2010-02-27T12:41:53Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:method=post}} {{#input:type=text|name=name}} {{#input:type=select|name=contribution| *one *two *three }} {{#formend:}} efb5af208bb652d2ba1ec4f20f79236470e1f7d3 395 394 2010-02-27T12:44:37Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:method=post}} Title: {{#input:type=text|name=dr}} Name: {{#input:type=text|name=name}} Affiliation: {{#input:type=text|name=affiliation}} Address: {{#input:type=textarea|rows=3}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=ajax|value=Post comment|update=wgBlogComments|onClick= var summary='comment posted by '+document.getElementById('blogName').value; document.getElementById('blogContent').setAttribute('value', '\n==='+document.getElementById('blogTitle').value+'===\n'+document.getElementById('blogBody').value+'\n:<i>'+summary+'</i>\n'); document.getElementById('blogSummary').setAttribute('value','Blog '+summary);}} {{#formend:}} 544dbaa6cab76bdfe9615f601f9cb159ed31cbe4 396 395 2010-02-27T12:45:01Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:method=post}} Title: {{#input:type=text|name=dr}} Name: {{#input:type=text|name=name}} Affiliation: {{#input:type=text|name=affiliation}} Address: {{#input:type=textarea|rows=3}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=ajax|value=Post comment|update=wgBlogComments|onClick= var summary='comment posted by '+document.getElementById('blogName').value; document.getElementById('blogContent').setAttribute('value', '\n==='+document.getElementById('blogTitle').value+'===\n'+document.getElementById('blogBody').value+'\n:<i>'+summary+'</i>\n'); document.getElementById('blogSummary').setAttribute('value','Blog '+summary);}} {{#formend:}} 355f93db337ff6f972bcf88109bc5cb819726428 397 396 2010-02-27T12:48:19Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:method=post}} Title: {{#input:type=text|name=dr}} Name: {{#input:type=text|name=name}} Affiliation: {{#input:type=text|name=affiliation}} Address: {{#input:type=textarea|rows=3}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#input:type=ajax|value=Post comment|update=wgBlogComments|onClick= var summary='comment posted by '+document.getElementById('blogName').value; document.getElementById('blogContent').setAttribute('value', '\n==='+document.getElementById('blogTitle').value+'===\n'+document.getElementById('blogBody').value+'\n:<i>'+summary+'</i>\n'); document.getElementById('blogSummary').setAttribute('value','Blog '+summary);}} {{#formend:}} a16ee5ab345ac90ac05ba036892ba4d515839bcf 398 397 2010-02-27T12:50:27Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:method=post}} Title: {{#input:type=text|name=dr}} Name: {{#input:type=text|name=name}} Affiliation: {{#input:type=text|name=affiliation}} Address: {{#input:type=textarea|rows=3}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} 3c370c940bab480cc57a3b5d43c59290e53c272e 399 398 2010-02-27T12:51:47Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:method=post}} Title:{{#input:type=text|name=dr}} Name: {{#input:type=text|name=name}} Affiliation: {{#input:type=text|name=affiliation}} Address: {{#input:type=textarea|rows=3}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} c2be4fbab343057e3b9cb607672fa2585dc6f927 400 399 2010-02-27T13:06:07Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form:action=<nowiki>http://camd04.ast.cam.ac.uk/~wyrzykow/exec/processform</nowiki>|method=post|}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} 8c434369f90c8a357ea9d50cc33cc8d52b63f46c 0 108 393 2010-02-27T12:29:24Z 86.9.207.4 0 Dummy article created for Simple Forms extension wikitext text/x-wiki Dummy article used by [http://www.mediawiki.org/wiki/Extension:Simple_Forms Extension:SimpleForms] 7e5b4a41c167c9e5ce85fbeae0fc1775f1021a83 0 103 401 374 2010-02-27T13:07:35Z Lukasz 2 wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Please register here to apply for an invitation.</big> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 5e1aa7a22186eae05f80655fc2e1a0f437010686 402 401 2010-02-27T13:07:55Z Lukasz 2 wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Registration is not open yet.</big> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. c51dd3e8ec3ef5b4d57de1f8942042251521f4c2 416 402 2010-02-28T23:26:59Z Lukasz 2 /* Registration */ wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Registration is not open yet.</big> <small>but if you really insist on seeing the registration form in its preliminary shape, go [[Workshop2010:registrationform | here]]</small> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 9dc6fa68afe5e5bcb8d2e833a9467d622fd4a36b 421 416 2010-03-01T12:12:56Z Lukasz 2 wikitext text/x-wiki =Registration= The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Registration is not open yet.</big> '''''If you already received an invitation you can relax and start planning you journey to Cambridge!''''' ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. bee5ae79d9ca8d072cffdea97b7d1bd9db23b22c 441 421 2010-03-03T15:10:07Z Lukasz 2 /* Registration */ wikitext text/x-wiki =Registration= == Invitees == <big>'''''If you already received an invitation please fill the form [[Workshop2010:registrationform | here]].''''</big> ---- == Application for an invitation == If you think you could contribute or benefit from attending the workshop, you have to apply for the invitation. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Registration is not open yet.</big> ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 577a0b5dd234979c3b58ddf5f44ce91e970434b8 442 441 2010-03-03T15:17:34Z Lukasz 2 wikitext text/x-wiki =Registration= == Invitees == <big>'''''If you already received an invitation please fill the form [[Workshop2010:registrationform | here]].'''</big> ---- == Application for an invitation == If you think you could contribute or benefit from attending the workshop, you have to apply for the invitation. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Registration is not open yet.</big> ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 28ba59da1b62d739b7212a9130c50de3b3de388e 443 442 2010-03-03T15:17:51Z Lukasz 2 wikitext text/x-wiki =Registration= == Invitees == <big>'''''If you already received an invitation please fill the form [[Workshop2010:registrationform | here]].'''''</big> ---- == Application for an invitation == If you think you could contribute or benefit from attending the workshop, you have to apply for the invitation. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. <big>Registration is not open yet.</big> ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 47b89acf187c133267667a2b66146cf49122ff58 447 443 2010-03-03T16:54:17Z Lukasz 2 /* Application for an invitation */ wikitext text/x-wiki =Registration= == Invitees == <big>'''''If you already received an invitation please fill the form [[Workshop2010:registrationform | here]].'''''</big> ---- == Application for an invitation == If you think you could contribute or benefit from attending the workshop, you have to apply for the invitation. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. '''Please fill the application form [[Workshop2010:applicationform|here]]'''. We accept the applications until the 30th of April 2010. ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 33309f489466f2ed5baf8105dac825ec3d4f97ef 448 447 2010-03-03T16:55:45Z Lukasz 2 /* Invitees */ wikitext text/x-wiki =Registration= == Invitees == <big>'''If you already received an invitation and wish to attend the workshop please fill the form [[Workshop2010:registrationform | here]].'''</big> Please do it by the 30th of April 2010. ---- == Application for an invitation == If you think you could contribute or benefit from attending the workshop, you have to apply for the invitation. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. '''Please fill the application form [[Workshop2010:applicationform|here]]'''. We accept the applications until the 30th of April 2010. ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. cb6bcbce71fb6b15c1ff7322c43b3406ad44bd2a 449 448 2010-03-03T17:06:48Z Lukasz 2 /* Application for an invitation */ wikitext text/x-wiki =Registration= == Invitees == <big>'''If you already received an invitation and wish to attend the workshop please fill the form [[Workshop2010:registrationform | here]].'''</big> Please do it by the 30th of April 2010. ---- == Application for an invitation == We welcome applications from all who would like to contribute to the workshop or who would benefit by their attendance. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. '''Please fill the application form [[Workshop2010:applicationform|here]]'''. We accept the applications until the 30th of April 2010. ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. 50ceb6c75ad007b985d743ef03f2671f599320bf 0 107 403 400 2010-02-28T14:48:20Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action="mailto:wyrzykow@gmail.com"|method=post|}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} e72accba50c1571f7662b11ec380bd165b359cfb 404 403 2010-02-28T14:55:32Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action="<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.pl</nowiki>" | method=post|}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} 817cad0020cd4efd4d02e2e2b2a59a5e29284d1d 405 404 2010-02-28T14:57:44Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action="<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki>" | method=post|}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} f7fc8980992ee13a1706b28701a1d6e940b286a5 406 405 2010-02-28T15:06:23Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action="<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki>" | method=post}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} f90bc43bbd14a1c02d4d9468c26604b692b78ee5 407 406 2010-02-28T15:32:31Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} b9b4ce53fb26a054b62c4013789bc7415fe7874b 408 407 2010-02-28T16:26:52Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.astrouw.edu.pl/~wyrzykow/exec/OLA/mailer.cgi</nowiki> | method=post}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} e144089b00563734845b9e614657345acad8ac11 409 408 2010-02-28T16:34:46Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=select|name=contribution| *one *two *three }} {{#input:type=submit|value=Send}} {{#formend:}} b9b4ce53fb26a054b62c4013789bc7415fe7874b 410 409 2010-02-28T16:54:05Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} Title: {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=30|style=width:auto|rows=1}} Address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=hidden|name=dupa}} {{#input:type=select|name=contribution| *none *talk *poster }} {{#input:type=submit|value=Send}} {{#formend:}} dbceadc166d0e55a38ab43e536b4068af2a9eb84 411 410 2010-02-28T17:37:08Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' Title (Mr/Mrs/Dr/Prof): {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} Work address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=hidden|name=wabik}} Telephone (with international dial code): {{#input:type=textarea|name=tel|rows=1|cols=20|style=width:auto}} Email: {{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} ---- {| |- | '''Your contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | Requested from date: | {{#input:type=textarea|name=accom_from|rows=1|cols=10|style=width:auto}} | Check-out date: | {{#input:type=textarea|name=accom_checkout|rows=1|cols=10|style=width:auto}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} ff0bc9a5ebfc4cf153f6a876439c47ed9493791e 412 411 2010-02-28T17:40:02Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' Title (Mr/Mrs/Dr/Prof): {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} Name: {{#input:type=textarea|name=name|cols=30|style=width:auto|rows=1}} Affiliation: {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} Work address: {{#input:type=textarea|rows=3|cols=30|style=width:auto}} {{#input:type=hidden|name=wabik}} Telephone (with international dial code): {{#input:type=textarea|name=tel|rows=1|cols=20|style=width:auto}} Email: {{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} ---- {| |- | '''Your contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | Requested from date: | {{#input:type=textarea|name=accom_from|rows=1|cols=10|style=width:auto}} | Check-out date: | {{#input:type=textarea|name=accom_checkout|rows=1|cols=10|style=width:auto}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 9b172192b241e1e8a0a4c5b6696ce52bf8bdf549 413 412 2010-02-28T23:24:14Z Lukasz 2 wikitext text/x-wiki Please '''do not fill the form yet''' as it is not working yet! ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''Your contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | Requested from date: | {{#input:type=textarea|name=accom_from|rows=1|cols=10|style=width:auto}} | Check-out date: | {{#input:type=textarea|name=accom_checkout|rows=1|cols=10|style=width:auto}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 1621a0215a823beb2954a4981b159e920cbb2fe6 414 413 2010-02-28T23:24:54Z Lukasz 2 wikitext text/x-wiki '''Registration is not yet open!''' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''Your contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | Requested from date: | {{#input:type=textarea|name=accom_from|rows=1|cols=10|style=width:auto}} | Check-out date: | {{#input:type=textarea|name=accom_checkout|rows=1|cols=10|style=width:auto}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 8d98cab7a4224a27b09bec786f31b61519db40c4 415 414 2010-02-28T23:25:10Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''Your contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | Requested from date: | {{#input:type=textarea|name=accom_from|rows=1|cols=10|style=width:auto}} | Check-out date: | {{#input:type=textarea|name=accom_checkout|rows=1|cols=10|style=width:auto}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} ad28dcfb6807980d8f8c20e86f675ee1ac3811af 417 415 2010-03-01T10:39:40Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | I am interested in accommodation in nearby Churchill College | {{#input:type=select|name=accom_churchill|*yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 8f1f2ad6a1a5173d037020cb15bab3d8289935f5 418 417 2010-03-01T10:57:16Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *none *talk *poster}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | I am interested in accommodation in nearby Churchill College | {{#input:type=select|name=accom_churchill|*yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Thursday 24th in one of the Cambridge colleges (King's, Trinity). The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner | {{#input:type=select|name=dinner| *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} d2e25aff869ced2abe316d432e90d7fba4efcaec 419 418 2010-03-01T11:00:26Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | I am interested in accommodation in nearby Churchill College | {{#input:type=select|name=accom_churchill|*yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Thursday 24th in one of the Cambridge colleges (King's, Trinity). The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner | {{#input:type=select|name=dinner| *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 87da27e35e56ea2d69dab60c6c22e17b90a835ad 420 419 2010-03-01T12:12:39Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' {| |- | I am interested in accommodation in nearby Churchill College | {{#input:type=select|name=accom_churchill|*yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner | {{#input:type=select|name=dinner| *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} e673900e3c7e3b43d87dfe71fad54b89e5d370f7 422 420 2010-03-01T12:58:27Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill|*yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner | {{#input:type=select|name=dinner| *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 193f51fa1b22ca39fb150022651ebcaeffef8f95 423 422 2010-03-01T13:00:21Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill|*yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} b2245965f8f183a2b04bbc14d0e0abe63da36a96 424 423 2010-03-01T13:55:09Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 29a1d3a88b48e74af0de7733b063a3b305e717cd 425 424 2010-03-01T13:55:32Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *Please select *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} 452abd62b3db3db59e5306bc5d5a2d29ce3547de 426 425 2010-03-01T14:05:20Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' | {{#input:type=select|name=contribution| *Please select *talk *poster *none}} |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=50|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=50|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single *double}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |- | Justification: | {{#input:type=textarea|name=support_justification|rows=3|cols=50|style=width:auto}} |} ---- {{#input:type=submit|value=Send}} {{#formend:}} a927dfa42576b1acad1eb5125ce3eced4fa754b8 427 426 2010-03-01T15:26:25Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel and accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=support_research|rows=6|cols=100|style=width:auto}} ''Brief (<250 words) justification of your need for financial support'' {{#input:type=textarea|name=support_justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} ad5f3634eb69bd5e8cfb79f90238cebac95b0d8c 428 427 2010-03-01T15:28:13Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=support_research|rows=6|cols=100|style=width:auto}} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=support_justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 847af85e848a3013026a35b5ee323a7bbb4942ac 429 428 2010-03-01T16:37:28Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *yes *no|value=no}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=support_justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 0acc132149eb87f2f702a99958f9685e10bd9260 430 429 2010-03-01T17:17:35Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=support_justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 5d0e09ce33450065796c89633cdd6771f6798a5a 431 430 2010-03-01T17:24:16Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 8de094d2aa766ce57b3f121ae15bcea968e2dec7 432 431 2010-03-01T17:48:04Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this application, please do not send it again!'''</big> <big>In order to amend you application please email ''gsaw2010@ast.cam.ac.uk'''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} f4985276e524b8c22ec6e6890d7001226f491254 433 432 2010-03-01T17:48:23Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this application, please do not send it again!'''</big> <big>In order to amend you application please email ''gsaw2010@ast.cam.ac.uk''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} da8538aeccc6af8cc2bfc9203da235e20e0012fe 434 433 2010-03-01T17:48:48Z Lukasz 2 wikitext text/x-wiki <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this application, please do not send it again!'''</big> <big>In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} dad864ad16983e892ce9993c1641dbeb347f0605 437 434 2010-03-03T13:45:00Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this form, please do not send it again!'''</big> <big>In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 44 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} cb4556b9e4310b7015651a2f33b4370d0daee149 444 437 2010-03-03T15:18:27Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this form, please do not send it again!'''</big> <big>In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 44 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 6dad1dbc3c98c867adee0b7c713bdc8a153db493 446 444 2010-03-03T16:44:52Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == <big>'''Registration is not yet open!'''</big> '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 42bc7f71d740979490092cb9cd2c69384c9e46ff 0 100 435 371 2010-03-03T12:57:19Z Lukasz 2 /* Important Dates */ wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' b30ad84ca139f683618191ab8d0cd3bd0390dc86 438 435 2010-03-03T14:41:39Z Lukasz 2 wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 75230827a77357326d58032b2ec16ea36ac3b2c6 0 109 436 2010-03-03T13:36:41Z Lukasz 2 Created page with '== Application for an invitation to the Workshop == <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this application, please do not send it agai...' wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is not yet open!'''</big> <big>'''If you have already send this application, please do not send it again!'''</big> <big>In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk''</big> ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's dinner on Wednesday 23th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} ebc11f10632c06615a15f3e2584812e26caae1f9 445 436 2010-03-03T16:44:06Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is not yet open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 7a9347c566f7f02a40a7e7b4001d7cfb4f5684bc 450 445 2010-03-04T10:49:47Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is not yet open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 388a3a1141269c71ce764bd3ae2586aaf25dec13 0 105 439 372 2010-03-03T14:42:42Z Lukasz 2 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 8b0f523ae12e18a370b703734244bfa7c664c80b 0 106 440 369 2010-03-03T14:56:08Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00 * Thursday 24 June - workshop's dinner with reception at Corpus Christi College (TBC) * Friday 25 June - workshop ends with lunch at 13:00 d3b3be8a44c70c8a69541ac1c40295769612c2e4 0 107 451 446 2010-03-04T10:50:06Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == <big>'''Registration is not yet open!'''</big> '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 3e763ff368fd1be45920c67a4bc06326d4e61472 462 451 2010-03-08T20:33:53Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 69bf1d058df3b21bf6e2f8cc56e1e74fe58bf049 470 462 2010-03-11T11:45:40Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 70a9578b3a4288518372f442c3a474103623ca0d 474 470 2010-03-12T16:06:10Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/06/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/06/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 3193e986efad9084dd8a25e31f44a180cf8e935d 0 105 452 439 2010-03-04T19:47:07Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchil1.jpg|right]] [[File:Churchil2.jpg|right]] Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens. The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries. Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge. If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 24bc8518fe2c5bb07f21b7470b5223292ee879ef 453 452 2010-03-04T19:47:30Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|right]] [[File:Churchill2.jpg|right]] Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens. The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries. Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge. If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 20d7e02c3a639cb1aa393867038867fb91988ae7 455 453 2010-03-04T19:50:19Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|300px|right]] [[File:Churchill2.jpg|right]] Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens. The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries. Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge. If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 9df6155c8450a33290739e297bd7cbea7933884a 456 455 2010-03-04T19:52:41Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|300px|right]] [[File:Churchill2.jpg|300px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. e8d55352a97e8d7400d665e5c85cf825ba0616d7 458 456 2010-03-04T19:54:49Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 7a8410737f562f9328ddb0b365497237bece5b76 459 458 2010-03-04T19:56:20Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 374e8d6b59e15d4c6850f2e7c13eb5af12435883 468 459 2010-03-10T17:46:49Z Lukasz 2 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.a1tourism.com/uk/cambridge-1.html Cambridge Lodge Hotel] (Hotel). == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 65a7ae6317c717fcb19b0cdbfab40e563f88152a 469 468 2010-03-10T17:47:48Z Lukasz 2 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus or 30m by train). Also not too far (approximately 1h 30m by bus) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (busses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are on-line. It may be better to book your bus ticket as soon as you know your flight details. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 2c3dccebb56ed1f0ee9b5467ce755c305230b6e1 6 110 454 2010-03-04T19:48:52Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 111 457 2010-03-04T19:53:59Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 100 460 438 2010-03-05T15:41:11Z Lukasz 2 wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' c47cabbd1962de7dce9049ede6b1dfe68b3cbf0a 480 460 2010-03-15T13:01:10Z Gaia 3 wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton * Laurent Eyer If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 8e8d6dc208906b8b4f6db368ed02e0bbb1a541b8 481 480 2010-03-15T13:09:44Z Gaia 3 wikitext text/x-wiki == Welcome! == Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 9ae2fad389430020887afb7bb154c7273ea786ae 488 481 2010-03-22T09:58:00Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web-poster.jpg|right]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 2f3c9bb231ed24e4ee5a438ea785814cce6d4316 490 488 2010-03-22T09:59:45Z Lukasz 2 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web.jpg|right|300px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' d0b8d410ce00d96a36c7f8a3514adcab548461ef 492 490 2010-03-22T10:01:19Z Lukasz 2 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web-poster.jpg|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 944713e82ac91912d0520dd6865e6d35532e44b4 493 492 2010-03-22T10:02:00Z Lukasz 2 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web-poster.jpg|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 3eb2695059e8df2d51c36235d867ef4d26e18167 496 493 2010-03-22T10:10:14Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web-poster.jpg|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * <big>[[workshop2010:poster|Workshop's poster for download]]</big> ---- === Workshop Organizing Committee === * Simon Hodgkin * Lukasz Wyrzykowski * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 82b95a013ec00f9531d5f5c2569a8f0e9d089211 497 496 2010-03-22T10:10:41Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web-poster.jpg|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * <big>[[workshop2010:poster|Workshop's poster for download]]</big> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 25ceac5af1cf9bc693f48e60c1be368ebff36a16 498 497 2010-03-22T10:10:49Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:GAIA-2010web-poster.jpg|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010. * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * <big>[[workshop2010:poster|Workshop's poster for download]]</big> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committe, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' fb347acf383ce684850c98fbdadb0eef5505e942 0 106 461 440 2010-03-05T16:04:13Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00 * Thursday 24 June - workshop's dinner with reception at Corpus Christi College * Friday 25 June - workshop ends in yearly afternoon. 743af56d9f5068270d86d3da92fb69dca0e6b181 485 461 2010-03-17T18:37:55Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00 * Thursday 24 June - workshop's dinner in one of the Cambridge colleges (TBC) * Friday 25 June - workshop ends in yearly afternoon. 25ee518dab716e8892f9ed15a9fb0268997794dd 486 485 2010-03-18T16:10:54Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00 * Thursday 24 June - workshop's dinner in one of the Cambridge colleges (TBC) * Friday 25 June - workshop ends in early afternoon. 6a54b5b475086658aeb8d3276e81422bb687a23b 0 109 463 450 2010-03-08T20:34:25Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is now open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in the Corpus Christi College. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} dbafa4ffd67f2f2144272db501e53cec49b780bf 471 463 2010-03-11T11:46:03Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is now open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/02/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/02/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 71fcb491796e41ccfdc5ed966d2d497d2039e7d7 475 471 2010-03-12T16:07:04Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is now open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/06/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/06/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Thursday 24th in one of the Cambridge colleges. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} a3a2582ac6636308019234eec477c41f85ef92e7 8 3 464 350 2010-03-09T14:27:58Z Gsawgwikiadmin 1 wikitext text/x-wiki * navigation ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2010 ** workshop2010:main|Main Workshop Page ** workshop2010:rationale|Rationale ** workshop2010:agenda|Agenda ** workshop2010:registration|Registration / Participants ** workshop2010:logistics|Logistics * SEARCH * TOOLBOX 552a210c6c6a418281487b6f3444d244296d1514 499 464 2010-03-22T13:10:52Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2010 ** workshop2010:main|Main Workshop Page ** workshop2010:rationale|Rationale ** workshop2010:agenda|Agenda ** workshop2010:registration|Registration / Participants ** workshop2010:logistics|Logistics * SEARCH * TOOLBOX a51dff095e1264a7a387b543aab8d341fed6ff87 0 103 465 449 2010-03-09T14:32:55Z Gsawgwikiadmin 1 wikitext text/x-wiki =Registration= == Invitees == <big>'''If you already received an invitation and wish to attend the workshop please fill the form [[Workshop2010:registrationform | here]].'''</big> Please do it by the 30th of April 2010. ---- == Application for an invitation == We welcome applications from all who would like to contribute to the workshop or who would benefit by their attendance. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, however can not guarantee it will be able to accommodate all applicants. '''Please fill the application form [[Workshop2010:applicationform|here]]'''. We accept the applications until the 30th of April 2010. ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. = Participants = List of registered [[Workshop2010:participants | participants]]. ca48666b7ae32d2fada756e0c90fb0d175361053 476 465 2010-03-12T16:20:14Z Lukasz 2 /* Application for an invitation */ wikitext text/x-wiki =Registration= == Invitees == <big>'''If you already received an invitation and wish to attend the workshop please fill the form [[Workshop2010:registrationform | here]].'''</big> Please do it by the 30th of April 2010. ---- == Application for an invitation == We welcome applications from all who would like to contribute to the workshop or who would benefit by their attendance. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, based on the description of their scientific interests and/or suggested contribution. '''Please fill the application form [[Workshop2010:applicationform|here]]'''. We accept the applications until the 30th of April 2010. ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. = Participants = List of registered [[Workshop2010:participants | participants]]. 6a820a2feb5d650abb70ce1c8e4dfd29d00c6b77 484 476 2010-03-17T18:36:31Z Lukasz 2 wikitext text/x-wiki =Registration= == Invitees == <big>'''If you already received an invitation and wish to attend the workshop please fill the form [[Workshop2010:registrationform | here]].'''</big> Please do it by the 30th of April 2010. ---- == Application for an invitation == We welcome applications from all who would like to contribute to the workshop or who would benefit by their attendance. The space of the meeting is limited to around 50 participants. The organizing committee will consider all applications from possible participants, based on the description of their scientific interests and/or suggested contribution. <big>'''Please fill the application form [[Workshop2010:applicationform|here]]'''.</big> We accept the applications until the 30th of April 2010. ---- [[File:great-esf-logo.png|right|200px]] Please note, there is '''no registration fee''' and the coffee/tea and lunches are free thanks to generous support of ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT]. GREAT provides also some limited support for researchers and students planning to attend the workshop. Funding can be applied for until '''30 April 2010'''. Please specify your needs in the application form above. = Participants = List of registered [[Workshop2010:participants | participants]]. ffd4f39a0aca0cf99f4af060996fa26cb29de2a3 0 50 466 340 2010-03-10T11:13:11Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra near maximum light resemble A-F absorption spectra of luminous stars at first * spectra at minimum light resemble spectra of Wolf-Rayet stars. * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days ---- Short transient searches in the other galaxies revealed possible new sub-class of novae: [http://uk.arxiv.org/abs/1003.1720 Kasliwal et al. 2010]. 324643d21add08c474ff80fc02805020b2de8ce9 467 466 2010-03-10T11:19:59Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra near maximum light resemble A-F absorption spectra of luminous stars at first * spectra at minimum light resemble spectra of Wolf-Rayet stars. * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days ---- Short transient searches in the other galaxies revealed possible new sub-class of novae: [http://uk.arxiv.org/abs/1003.1720 Kasliwal et al. 2010]. They usually stay above the Gaia detection limit for not more than 10 days. ea56b55ce4877753a642ef39c25dd6115feb0d2d 0 112 472 2010-03-11T11:48:08Z Lukasz 2 Created page with '* Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast' wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast 8f3277706a767933d632eaac12f175524f868e48 473 472 2010-03-12T16:05:39Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech b14f6e3b9e3c13fcc1ccc88dbee661cf622fe24d 477 473 2010-03-15T09:52:25Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University 366df53ca49353ee761feb8d7d3fddbb06e8186a 478 477 2010-03-15T09:52:55Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos 9e9e81234a2f8931bd05ec5129946810438474d3 479 478 2010-03-15T12:42:45Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos * Dr. Mark Sullivan, Oxford 55f7e36fdc4d35ea170a41d25eb415e12191d37a 482 479 2010-03-16T12:36:06Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos * Dr. Mark Sullivan, Oxford * Dr. Laurent Eyer, Geneva * Dr. Martin Dominik, St.Andrews da5a653b49ff315ab8b5e5fba026f9debdafe597 483 482 2010-03-17T17:36:39Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos * Dr. Mark Sullivan, Oxford * Dr. Laurent Eyer, Geneva * Dr. Martin Dominik, St.Andrews * Dr. Massimo Turatto, Catania 041e888b907cb371e178783727a92347eccbbc93 487 483 2010-03-18T16:25:56Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos * Dr. Mark Sullivan, Oxford * Dr. Laurent Eyer, Geneva * Dr. Martin Dominik, St.Andrews * Dr. Massimo Turatto, Catania * Prof. Lech Mankiewicz, PAN Warsaw f8b5c28c9d39f285085db973602811b6acb10417 6 113 489 2010-03-22T09:58:19Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 114 491 2010-03-22T09:59:58Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 115 494 2010-03-22T10:09:04Z Lukasz 2 Created page with '[[File:GAIA-2010web-poster.jpg|right|400px]] <big>Choose the right format of the poster </big> * [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster-small....' wikitext text/x-wiki [[File:GAIA-2010web-poster.jpg|right|400px]] <big>Choose the right format of the poster </big> * [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster-small.jpg Small] * http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster.jpg Big (A4)] We would appreciate if you could print the A4 version and display in your institute. 379625a7b49148a50cba84eb700c29b97280f862 495 494 2010-03-22T10:09:19Z Lukasz 2 wikitext text/x-wiki [[File:GAIA-2010web-poster.jpg|right|400px]] <big>Choose the right format of the poster </big> * [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster-small.jpg Small] * [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster.jpg Big (A4)] We would appreciate if you could print the A4 version and display in your institute. a7048b4038c5f68891cef9a590f6ee0289bd1f3b 500 495 2010-03-22T15:19:56Z Lukasz 2 wikitext text/x-wiki [[File:GAIA-2010web-poster.jpg|right|400px]] <big>Choose the right format of the poster </big> * [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster-small.jpg Small] * [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/GaiaWorkshop2010poster.jpg Big (A4)] We would appreciate if you could print the A4 version and display in your institution. 91289b0d131dd82935571884b2eea9e4444545f1 0 11 501 22 2010-03-23T10:48:32Z Lukasz 2 wikitext text/x-wiki Main aim of the Verification Phase is to verify the robustness of the issued alerts and confirm them with the dedicated set of follow-up telescopes available for ''Target of Opportunity'' (ToO) mode. This should reveal all necessary adjustments to be done in the detection algorithm to assure the best and the most robust performance later on. Verification Phase will last for 2-3 months and is planned to take place as early in the mission as possible, as soon as the alerting system is ready to perform. Currently, it seems it will happen only after the first cycle (half a year, i.e. late 2012/early 2013), as the accumulated data ("baseline flux") will not be available before. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Loiano || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Bologna, Italy |- |Konkoly || Laszlo Szabados (szabados@szombat.konkoly.hu) || |- |} 6dd0a3137482f6952caf46ba80be886e719725ee 508 501 2010-03-25T10:03:12Z Laszlo.szabados 18 details of the available telescopes at the Konkoly Observatory wikitext text/x-wiki Main aim of the Verification Phase is to verify the robustness of the issued alerts and confirm them with the dedicated set of follow-up telescopes available for ''Target of Opportunity'' (ToO) mode. This should reveal all necessary adjustments to be done in the detection algorithm to assure the best and the most robust performance later on. Verification Phase will last for 2-3 months and is planned to take place as early in the mission as possible, as soon as the alerting system is ready to perform. Currently, it seems it will happen only after the first cycle (half a year, i.e. late 2012/early 2013), as the accumulated data ("baseline flux") will not be available before. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Loiano || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Bologna, Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} dca0db63e2c3d8f12240c0d2c56a13079dfdc804 0 102 502 356 2010-03-23T11:07:41Z Gsawgwikiadmin 1 /* Target participants: */ wikitext text/x-wiki = Workshop's Rationale = Gaia will repeatedly monitor the whole sky in the optical. The Gaia Science Alerts stream therefore represents a unique opportunity, and holds a significant responsibility. Triggers from transient phenomena are the first data that the astronomical community will see from the satellite. It is up the Gaia Science Alerts Team to make sure that the alert stream is accurate, reliable, interesting and free from (or at least acceptably low in) contamination. It is vital to make sure that the astronomical community is ready for these Gaia alerts, and that Gaia starts delivering science quickly. In addition, we will raise public awareness about (and involvement with) the satellite very early on in the mission. == The motivation for the workshop: == * To focus community attention on the scientific possibilities that will arise from the Gaia Science Alerts data stream, and to make sure that astronomers are prepared and motivated to exploit the data as it arrives. * To invite the community to influence the scope of the science alerts processing algorithms and alert strategies, to ensure that returns from the mission are maximized, and that exciting opportunities are not overlooked. == Target participants: == # Experts on the Gaia mission and data flow system, together with developers and scientists working on the Science Alerts System. # Astronomers who are actively involved or interested in ongoing or planned surveys for transient phenomena, for example the Palomar Transient Factory, the Catalina Survey, the Supernova Factory, PanSTARRS, LSST, WASP, OGLE, ASAS. # Active researchers into transient phenomena, such as Supernovae, Microlensing Events, Gamma Ray Bursts, Classical Novae, ExtraGalactic variability, CVs, Be stars, massive stars, solar system objects and so on. # Scientists who are involved in the distribution of Alert information, e.g. from eSTAR and GCN # Individuals who are interested in the outreach possibilities of Gaia Science Alerts. 13c3ceb928196f7f476621a85b799d88d001bc4d 531 502 2010-04-19T11:01:49Z Lukasz 2 wikitext text/x-wiki = Workshop's Rationale = The main aim of the workshop is to focus community attention on and involvement in the scientific possibilities that will arise from the Gaia Science Alerts data stream. Gaia will be launched in 2012 and will repeatedly monitor the whole sky in the optical during its 5 year mission. The Gaia Science Alerts team will search for transient phenomena in source photometry as the data are promptly ingested for processing. The aim will be to detect large numbers of Supernovae, Microlensing Events, Novae, Gamma-Ray Burst afterglows, and other interesting transient or anomalous phenomena. Gaia Alerts will be released to the world-wide community to enable rapid follow-up of the transients. The purpose of the workshop is to discuss in detail the expected nature and potential of the Gaia Science Alerts data stream. Our goals are: * To develop a roadmap for the coordination and preparation of ground based verification and follow-up observing campaigns. * Identification of the most exciting targets of opportunity for the Gaia Science Alerts stream. * Improved understanding of the expected events and contaminants rates for Gaia alerts. * Improved requirements on the development and operation of the Gaia Alerts stream, including time-scales, sensitivity, acceptable contamination rates and so on. Gaia Alerts represent a unique opportunity: triggers from transient phenomena are the first data that the astronomical community will see from the satellite. == Target participants: == We aim to bring together, in an interactive workshop environment, astronomers working in key relevant areas: * Experts on the Gaia mission and data flow system, together with developers and scientists working on the Science Alerts System. * Astronomers who are actively involved or interested in ongoing or planned surveys for transient phenomena, for example the Palomar Transient Factory, the Catalina Survey, the Supernova Factory, PanSTARRS, LSST, WASP, OGLE, ASAS. * Active researchers into transient phenomena, such as Supernovae, Microlensing Events, Gamma Ray Bursts, Classical Novae, ExtraGalactic variability, CVs, Be stars, massive stars, solar system objects and so on. * Scientists who are involved in the distribution of Alert information, e.g. from eSTAR and GCN * Individuals who are interested in the outreach possibilities of Gaia Science Alerts. e4c069032126e95188103797969674d81be7c177 534 531 2010-04-19T11:03:35Z Lukasz 2 wikitext text/x-wiki = Workshop's Rationale = The main aim of the workshop is to focus community attention on and involvement in the scientific possibilities that will arise from the Gaia Science Alerts data stream. Gaia will be launched in 2012 and will repeatedly monitor the whole sky in the optical during its 5 year mission. The Gaia Science Alerts team will search for transient phenomena in source photometry as the data are promptly ingested for processing. The aim will be to detect large numbers of Supernovae, Microlensing Events, Novae, Gamma-Ray Burst afterglows, and other interesting transient or anomalous phenomena. Gaia Alerts will be released to the world-wide community to enable rapid follow-up of the transients. The purpose of the workshop is to discuss in detail the expected nature and potential of the Gaia Science Alerts data stream. Our goals are: * To develop a roadmap for the coordination and preparation of ground based verification and follow-up observing campaigns. * Identification of the most exciting targets of opportunity for the Gaia Science Alerts stream. * Improved understanding of the expected events and contaminants rates for Gaia alerts. * Improved requirements on the development and operation of the Gaia Alerts stream, including time-scales, sensitivity, acceptable contamination rates and so on. Gaia Alerts represent a unique opportunity: triggers from transient phenomena are the first data that the astronomical community will see from the satellite. == Target participants: == We aim to bring together, in an interactive workshop environment, astronomers working in key relevant areas: * Experts on the Gaia mission and data flow system, together with developers and scientists working on the Science Alerts System. * Astronomers who are actively involved or interested in ongoing or planned surveys for transient phenomena, for example the Palomar Transient Factory, the Catalina Survey, the Supernova Factory, PanSTARRS, LSST, WASP, OGLE, ASAS. * Active researchers into transient phenomena, such as Supernovae, Microlensing Events, Gamma Ray Bursts, Classical Novae, ExtraGalactic variability, CVs, Be stars, massive stars, solar system objects and so on. * Scientists who are involved in the distribution of Alert information, e.g. from eSTAR and GCN * Individuals who are interested in the outreach possibilities of Gaia Science Alerts. We view this meeting as a kickoff for collaborative work to plan pre-launch and mission-based activities. 47e5a352bd35c75efd52b30993fe036611d19f83 0 10 503 341 2010-03-23T11:14:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] cf58ac9f6920b3560af04cdbda50f3c1bded8fda 0 9 504 232 2010-03-23T12:03:11Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with the possible alerts, which are not interesting enough for rapid follow-up. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum.''' ===Possible triggers for Science Alerts=== * [[Triggers:LPVs | Long period variables]] * [[Triggers:AGN | Active Galactic Nuclei (AGNs, Quasars, QSOs)]] 9e3f5dbd0414a227c05598a4fb48e640c7f704a4 0 8 505 331 2010-03-23T12:04:58Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:Supernovae | Supernovae]] * [[Triggers:TTau | T Tauri type pre-main sequence stars]] * [[Triggers:XBs | X-ray binaries (XBs)]] * [[Triggers:Other | Other rare transients]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 9a9d5baed90937939fbf4c5bae29b4a10e01eb52 0 112 506 487 2010-03-24T10:40:28Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos * Dr. Mark Sullivan, Oxford * Dr. Laurent Eyer, Geneva * Dr. Martin Dominik, St.Andrews * Dr. Massimo Turatto, Catania * Prof. Lech Mankiewicz, PAN Warsaw * Mr. Marcin Wardak, Warsaw * Dr. Dovi Poznanski, Berkeley bff035913b0b6babd87748636e1fd61bc7c5e294 520 506 2010-03-31T11:02:03Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast * Dr. Yael Naze, University of Liege * Dr. Ashish Mahabal, Caltech * Prof. Andy Gould, Ohio State University * Dr. Przemek Wozniak, Los Alamos * Dr. Mark Sullivan, Oxford * Dr. Laurent Eyer, Geneva * Dr. Martin Dominik, St.Andrews * Dr. Massimo Turatto, Catania * Prof. Lech Mankiewicz, PAN Warsaw * Mr. Marcin Wardak, Warsaw * Dr. Dovi Poznanski, Berkeley * Dr. Paolo Tanga, Nice 274ec0549f26ebef6ef4643474fa37485954f2a7 521 520 2010-03-31T14:53:56Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester, UK * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast, UK * Dr. Yael Naze, University of Liege, Belgium * Dr. Ashish Mahabal, Caltech, US * Prof. Andy Gould, Ohio State University, US * Dr. Przemek Wozniak, Los Alamos, US * Dr. Mark Sullivan, Oxford, UK * Dr. Laurent Eyer, Geneva, Switzerland * Dr. Martin Dominik, St.Andrews, UK * Dr. Massimo Turatto, Catania, Italy * Prof. Lech Mankiewicz, PAN Warsaw, Poland * Mr. Marcin Wardak, Warsaw, Poland * Dr. Dovi Poznanski, Berkeley, US * Dr. Paolo Tanga, Nice, France * Dr. Avishay Gal-Yam, Weizmann, Israel c0909ae6410a76127905b5f6e6c06e60f04fc835 522 521 2010-04-06T10:04:48Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester, UK * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast, UK * Dr. Yael Naze, University of Liege, Belgium * Dr. Ashish Mahabal, Caltech, US * Prof. Andy Gould, Ohio State University, US * Dr. Przemek Wozniak, Los Alamos, US * Dr. Mark Sullivan, Oxford, UK * Dr. Laurent Eyer, Geneva, Switzerland * Dr. Martin Dominik, St.Andrews, UK * Dr. Massimo Turatto, Catania, Italy * Prof. Lech Mankiewicz, PAN Warsaw, Poland * Mr. Marcin Wardak, Warsaw, Poland * Dr. Dovi Poznanski, Berkeley, US * Dr. Paolo Tanga, Nice, France * Dr. Avishay Gal-Yam, Weizmann, Israel * Prof. Iain Steele, Liverpool, UK 62cb131f25ab8f382fbff32a35ffb0981425bc02 523 522 2010-04-11T18:35:02Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester, UK * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast, UK * Dr. Yael Naze, University of Liege, Belgium * Dr. Ashish Mahabal, Caltech, US * Prof. Andy Gould, Ohio State University, US * Dr. Przemek Wozniak, Los Alamos, US * Dr. Mark Sullivan, Oxford, UK * Dr. Laurent Eyer, Geneva, Switzerland * Dr. Martin Dominik, St.Andrews, UK * Dr. Massimo Turatto, Catania, Italy * Prof. Lech Mankiewicz, PAN Warsaw, Poland * Mr. Marcin Wardak, Warsaw, Poland * Dr. Dovi Poznanski, Berkeley, US * Dr. Paolo Tanga, Nice, France * Dr. Avishay Gal-Yam, Weizmann, Israel * Prof. Iain Steele, Liverpool, UK * Dr. Martin Altmann, Heidelberg, Germany 24e683b958d06ba74eca116d942043ffdb07fbf4 524 523 2010-04-12T11:01:20Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester, UK * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast, UK * Dr. Yael Naze, University of Liege, Belgium * Dr. Ashish Mahabal, Caltech, US * Prof. Andy Gould, Ohio State University, US * Dr. Przemek Wozniak, Los Alamos, US * Dr. Mark Sullivan, Oxford, UK * Dr. Laurent Eyer, Geneva, Switzerland * Dr. Martin Dominik, St.Andrews, UK * Dr. Massimo Turatto, Catania, Italy * Prof. Lech Mankiewicz, PAN Warsaw, Poland * Mr. Marcin Wardak, Warsaw, Poland * Dr. Dovi Poznanski, Berkeley, US * Dr. Paolo Tanga, Nice, France * Dr. Avishay Gal-Yam, Weizmann, Israel * Prof. Iain Steele, Liverpool, UK * Dr. Martin Altmann, Heidelberg, Germany * Dr Elena Pancino, Bologna, Italy * Prof. Michel Dennefeld, Paris, France bdb99484a918f33544f3c74befb6b5601202e963 527 524 2010-04-12T16:05:03Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester, UK * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast, UK * Dr. Yael Naze, University of Liege, Belgium * Dr. Ashish Mahabal, Caltech, US * Prof. Andy Gould, Ohio State University, US * Dr. Przemek Wozniak, Los Alamos, US * Dr. Mark Sullivan, Oxford, UK * Dr. Laurent Eyer, Geneva, Switzerland * Dr. Martin Dominik, St.Andrews, UK * Dr. Massimo Turatto, Catania, Italy * Prof. Lech Mankiewicz, PAN Warsaw, Poland * Mr. Marcin Wardak, Warsaw, Poland * Dr. Dovi Poznanski, Berkeley, US * Dr. Paolo Tanga, Nice, France * Dr. Avishay Gal-Yam, Weizmann, Israel * Prof. Iain Steele, Liverpool, UK * Dr. Martin Altmann, Heidelberg, Germany * Dr Elena Pancino, Bologna, Italy * Prof. Michel Dennefeld, Paris, France * Dr. Eran Ofek, Caltech, US 781549aaac1698fb258b0eb1cd7e85e2d4fe6e04 528 527 2010-04-13T16:01:46Z Lukasz 2 wikitext text/x-wiki * Prof. Paul O'Brien, University of Leicester, UK * Dr. Timo Prusti, ESA * Prof. Stephen Smartt, Queen's University Belfast, UK * Dr. Yael Naze, University of Liege, Belgium * Dr. Ashish Mahabal, Caltech, US * Prof. Andy Gould, Ohio State University, US * Dr. Przemek Wozniak, Los Alamos, US * Dr. Mark Sullivan, Oxford, UK * Dr. Laurent Eyer, Geneva, Switzerland * Dr. Martin Dominik, St.Andrews, UK * Dr. Massimo Turatto, Catania, Italy * Prof. Lech Mankiewicz, PAN Warsaw, Poland * Mr. Marcin Wardak, Warsaw, Poland * Dr. Dovi Poznanski, Berkeley, US * Dr. Paolo Tanga, Nice, France * Dr. Avishay Gal-Yam, Weizmann, Israel * Prof. Iain Steele, Liverpool, UK * Dr. Martin Altmann, Heidelberg, Germany * Dr Elena Pancino, Bologna, Italy * Prof. Michel Dennefeld, Paris, France * Dr. Eran Ofek, Caltech, US * Dr. Danny Steeghs, Warwick, UK 3af8b268f7e4a17fd359160afdb03afbeb212ffd 529 528 2010-04-13T16:51:07Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr. Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr. Yael Naze, University of Liege, Belgium # Dr. Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr. Przemek Wozniak, Los Alamos, US # Dr. Mark Sullivan, Oxford, UK # Dr. Laurent Eyer, Geneva, Switzerland # Dr. Martin Dominik, St.Andrews, UK # Dr. Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr. Marcin Wardak, Warsaw, Poland # Dr. Dovi Poznanski, Berkeley, US # Dr. Paolo Tanga, Nice, France # Dr. Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr. Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr. Eran Ofek, Caltech, US # Dr. Danny Steeghs, Warwick, UK 1103064c58e56d64ffbbbe61fc8360e28f4f46d8 530 529 2010-04-16T09:19:28Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic 7ee79f6c0f72f64659b6c40b03da0813900346c8 535 530 2010-04-19T15:03:08Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK 1bca17928d83807bea8ffe1403a6eb2b888954b4 536 535 2010-04-21T10:11:24Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy 81f84c8811039c6722af46189a98569c0c3e8257 537 536 2010-04-22T08:42:22Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland 1f24af69fd801c60d85c07f36b13d72489f0bd80 538 537 2010-04-22T11:59:45Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic 950700b2d6b5eb44b2e52dee24bfaaa3dfd8f256 540 538 2010-04-26T09:23:51Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain bfae7d93a06d62b07b29f28c896e4cb4f21c6897 541 540 2010-04-26T10:59:10Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain 9537ca6103c58f75402f8bc7f5fc7958c64a4634 542 541 2010-04-28T09:03:59Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK 62f6b28aee2aa6c863d682df2d901f26b6720cdd 543 542 2010-04-28T15:37:18Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK 97ee3ccc38d6f82a9234387eaa90ac6f131abd1b 544 543 2010-04-29T14:48:28Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK 57a9608ca48936479bc084b76091d5c0358476a6 545 544 2010-04-30T16:03:01Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia a0a9b35b50af2be7165c7b97e3bce94e338d4604 550 545 2010-05-07T12:56:24Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Enrico Cappellaro, Padova, Italy # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK b09b8b6f65be5cb5926c7f6f04e3469449fb8170 0 17 507 324 2010-03-25T09:29:29Z Lukasz 2 wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == '''The list here will contain surveys probable to be in operation from 2012 to 2017 suitable for following-up Gaia alerts. Please expand it with more surveys.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * * * a334f4a3abb27e70e5cd6ac9eb4c452270bafdaa 509 507 2010-03-25T10:07:40Z Laszlo.szabados 18 list of telescopes available at the Konkoly Observatory wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == '''The list here will contain surveys probable to be in operation from 2012 to 2017 suitable for following-up Gaia alerts. Please expand it with more surveys.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * a332bf4b3e044927a81f09ed021c85812f578643 510 509 2010-03-25T10:11:35Z Laszlo.szabados 18 list of telescopes available at the Konkoly Observatory wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == '''The list here will contain surveys probable to be in operation from 2012 to 2017 suitable for following-up Gaia alerts. Please expand it with more surveys.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * d2f2ed3a91cde5eda526c56f38b0bee787661c76 511 510 2010-03-25T10:36:42Z Lukasz 2 wikitext text/x-wiki == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 3030479feae4530ba0070cfadfaae82e86e4d01c 0 106 512 486 2010-03-25T13:54:58Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00, evening: workshop's dinner in the college * Thursday 24 June * Friday 25 June - workshop ends in early afternoon. 7d8bd2d8c325722e8fb466e8ef6d84370f90a30d 517 512 2010-03-30T10:09:41Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * Wednesday 23 June - workshop starts with coffee at 11:00, evening: reception and workshop's dinner in the Churchill college * Thursday 24 June * Friday 25 June - workshop ends in early afternoon. ca764f4f5d0a5258539befce9e8679dcf655bac8 518 517 2010-03-30T10:10:15Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= * '''Wednesday 23 June''' - workshop starts with coffee at 11:00, evening: reception and workshop's dinner in the Churchill college * '''Thursday 24 June''' * '''Friday 25 June''' - workshop ends in early afternoon. d2bb4754bcd704c641db1a5e21c0741a89565d7d 532 518 2010-04-19T11:03:05Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion period. We anticipate stimulating significant discussion and tackling the goals of the workshop. We view this meeting as a kickoff for collaborative work to plan pre-launch and mission-based activities. * '''Wednesday 23 June''' - workshop starts with coffee at 11:00, evening: reception and workshop's dinner in the Churchill college * '''Thursday 24 June''' * '''Friday 25 June''' - workshop ends in early afternoon. 286158ed6493e65c860829354e450cf09fa4f9e8 533 532 2010-04-19T11:03:15Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion period. We anticipate stimulating significant discussion and tackling the goals of the workshop. * '''Wednesday 23 June''' - workshop starts with coffee at 11:00, evening: reception and workshop's dinner in the Churchill college * '''Thursday 24 June''' * '''Friday 25 June''' - workshop ends in early afternoon. 62df93f4c8ce0e715921da036e0ea1e60690b573 0 107 513 474 2010-03-25T13:57:04Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/06/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/06/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Wednesday 23th in the college. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 472cbb2b004faf63236a314639f79a24803c012c 525 513 2010-04-12T15:37:19Z Lukasz 2 wikitext text/x-wiki == Registration form for invitees == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/06/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/06/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on'' '''''Wednesday 23th''''' ''in the college. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 786d6430e9f807f3fb723a8ae431a65dd7abde35 0 109 514 475 2010-03-25T13:57:32Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is now open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/06/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/06/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on Wednesday 23th in the college. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 4545b8f2664a49b821e00130f2d7026d60079eac 526 514 2010-04-12T15:37:44Z Lukasz 2 wikitext text/x-wiki == Application for an invitation to the Workshop == <big>'''Registration is now open!'''</big> '''If you have already received an invitation, please fill the registration form [[Workshop2010:registrationform|here]].''' '''If you have already send this application, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2010@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation my self}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=23/06/2010}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=25/06/2010}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 60 GBP per night *twin at 75 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner'' '''''Wednesday 23th''''' ''in the college. The estimated cost would be 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in euros).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} e337b45f2cc468669f7e96d4ae117cd51c8010e5 0 100 515 498 2010-03-29T09:54:55Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * <big>[[workshop2010:poster|Workshop's poster for download]]</big> [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' df72801be4cec50b5ea08b1b0608e60398a36d0e 547 515 2010-05-04T11:29:25Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 25cfbd54e56d0209f53f736b95e1efe4cf90b51a 548 547 2010-05-04T11:29:48Z Lukasz 2 /* Workshop Organizing Committee */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski (head) * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' d5a3b4b8ea42e494e5de7ab9332052a52f7a3371 549 548 2010-05-04T11:30:06Z Lukasz 2 /* Workshop Organizing Committee */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Registration]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' d3fbeb968c1f96dbd378e036cf05acc5dc04c461 0 50 516 467 2010-03-30T09:43:25Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra near maximum light resemble A-F absorption spectra of luminous stars at first * spectra at minimum light resemble spectra of Wolf-Rayet stars. * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present Exemplary observations of a very fast nova with 0.3m Meade telescope: [[http://uk.arxiv.org/abs/1003.5371 Munari and Dallaporta]]. '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days ---- Short transient searches in the other galaxies revealed possible new sub-class of novae: [http://uk.arxiv.org/abs/1003.1720 Kasliwal et al. 2010]. They usually stay above the Gaia detection limit for not more than 10 days. ebde8ad710bd9bd2cfe2ecb3d94ebf275d8b9e68 539 516 2010-04-23T12:02:22Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is roughly 30 novae per year in the Milky Way and about 20 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra near maximum light resemble A-F absorption spectra of luminous stars at first * spectra at minimum light resemble spectra of Wolf-Rayet stars. * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present Exemplary observations of a very fast nova with 0.3m Meade telescope: [[http://uk.arxiv.org/abs/1003.5371 Munari and Dallaporta]]. '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days ---- Short transient searches in the other galaxies revealed possible new sub-class of novae: [http://uk.arxiv.org/abs/1003.1720 Kasliwal et al. 2010]. They usually stay above the Gaia detection limit for not more than 10 days. ---- Interesting paper on classification and properties of novae: [[http://uk.arxiv.org/abs/1004.3698 Strope, Schaefer & Henden 2010]] 3ff5b44a1c6376412ee8c37a651b1418490f9ca0 6 113 519 489 2010-03-30T14:58:29Z Lukasz 2 uploaded a new version of "[[File:GAIA-2010web-poster.jpg]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 103 546 484 2010-05-04T11:28:29Z Lukasz 2 wikitext text/x-wiki =Registration= <center><big><big>'''Registration is now closed.'''</big></big></center> Please contact the organizers at ''gsaw2010@ast.cam.ac.uk'' if you have any queries regarding the registration. ---- = Participants = List of registered [[Workshop2010:participants | participants]]. 35ed04bcbf37773e634b55c09c7acbdf3f623257 0 112 551 550 2010-05-10T09:54:50Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Enrico Cappellaro, Padova, Italy # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK a4c175de89199c3faf2b3e7cb3fdfd770d7c4efc 552 551 2010-05-10T12:52:20Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Enrico Cappellaro, Padova, Italy # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK ed1abfc3257c414b978500f7842d098d4bce8a30 557 552 2010-05-14T13:28:02Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Enrico Cappellaro, Padova, Italy # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK dcdacb9c54b4c45f52c5bb443f20ccf977197ae1 558 557 2010-05-17T18:39:18Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Enrico Cappellaro, Padova, Italy # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France 81de04547ccc6ea4bb8ba7c2bc84b0c6c1ad328a 560 558 2010-05-18T22:01:05Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Enrico Cappellaro, Padova, Italy # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France a3628dd7fbffc41de4f9fdc6ec6851294ab14196 561 560 2010-05-19T08:22:16Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France 18d367bb2d10888932459d6eaebd37a2932ceffa 564 561 2010-05-26T11:28:10Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Prof Martin C. Smith, Kavli, Beijing c8d0420bfc4b4ca70818c4f55c085c01acda71b5 574 564 2010-06-03T17:03:20Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Prof Martin C. Smith, Kavli, Beijing # Dr Lukasz Wyrzykowski, IoA, UK 5fb787a3a2ef4530e053e06e9a6f0353f9bbedca 577 574 2010-06-04T10:40:36Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK 9903bed729d746836697dc0e324f386b87f30ffb 580 577 2010-06-04T14:15:58Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK # Dr Sergey Koposov, IoA, UK c08bf897814f9a5f09088798d71b86403793bbfe 581 580 2010-06-04T15:01:35Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK # Dr Sergey Koposov, IoA, UK # Dr Simon Hodgkin, IoA, UK 4c8d41378caad579e3d881a2d0b943c54b1cd617 582 581 2010-06-07T14:27:13Z Lukasz 2 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Dr Elena Pancino, Bologna, Italy # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK # Dr Sergey Koposov, IoA, UK # Dr Simon Hodgkin, IoA, UK # Dr Nami Mowlavi, Geneva, Switzerland 6369e9de4d11f78bf6b052d024f4628140b728fc 598 582 2010-06-18T09:24:16Z Sth 6 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK # Dr Sergey Koposov, IoA, UK # Dr Simon Hodgkin, IoA, UK # Dr Nami Mowlavi, Geneva, Switzerland # Professor Tim Naylor, Exeter, UK d81d1107c28a9215ffe2d787220c651a6dba527f 599 598 2010-06-18T09:24:50Z Sth 6 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK # Dr Sergey Koposov, IoA, UK # Dr Simon Hodgkin, IoA, UK # Dr Nami Mowlavi, Geneva, Switzerland # Professor Tim Naylor, Exeter, UK 18e7abc0eea440686a37cf75a66a36ac33bac8c7 0 10 553 503 2010-05-12T12:08:35Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. [[gaia_scanning_anim.mp4 | Here]] you can download a movie showing Gaia scanning law and how number of observations per star is growing over the entire sky. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 3647e609cc710b4b58a3f8820120aeb7c6f70bd3 554 553 2010-05-12T12:09:13Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. [[Media:gaia_scanning_anim.mp4 | Here]] you can download a movie showing Gaia scanning law and how number of observations per star is growing over the entire sky. == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 4f935cce9d72b0030a2e45f7a7d7f864c14997da 555 554 2010-05-12T12:12:23Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim.mp4 Here]] you can download a movie (40MB) showing Gaia scanning law and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 1e631e2b70508e169896882ac7411011b524974c 556 555 2010-05-12T12:12:52Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim.mp4 Here] you can download a movie (40MB) showing Gaia scanning law and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 389b1ed76200e3ad58dc21e66068cfe1f5274c02 559 556 2010-05-18T10:50:24Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** G-flux observations - all available in given cycle ** accumulated G-flux: mean and scatter ** accumulated BP and RP colours ** low-dispersion BP and RP spectrometry ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] d940387d7b4549495b2abf56ac496159a2d3e0d7 575 559 2010-06-04T10:37:06Z Lukasz 2 /* Detection */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** newly acquired G-flux observations, 8-9 measurements separated by 4.4s (per-CCD) ** historical G-flux observations ** mean BP and RP colours ** low-dispersion BP and RP spectrometry (raw,uncalibrated) ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] e206fbb3bc2c44824b92d92f8c99d7534481aff3 576 575 2010-06-04T10:40:18Z Lukasz 2 /* Sampling properties of Gaia */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system. ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** newly acquired G-flux observations, 8-9 measurements separated by 4.4s (per-CCD) ** historical G-flux observations ** mean BP and RP colours ** low-dispersion BP and RP spectrometry (raw,uncalibrated) ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. [[File:gog_sampling.png|200px|left|thumb|Sampling distribution over the whole sky from Gaia simulator]] On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] c91af5848dc8ed5acd801eb9b3678e59de1f8911 579 576 2010-06-04T11:24:11Z Lukasz 2 /* General */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system (from December 2009, not completely up-to-date). ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** newly acquired G-flux observations, 8-9 measurements separated by 4.4s (per-CCD) ** historical G-flux observations ** mean BP and RP colours ** low-dispersion BP and RP spectrometry (raw,uncalibrated) ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. [[File:gog_sampling.png|200px|left|thumb|Sampling distribution over the whole sky from Gaia simulator]] On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 6aaa6cdc7e869ffb252c0f1d5405a8265cbf1417 0 106 562 533 2010-05-21T13:19:13Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion period. We anticipate stimulating significant discussion and tackling the goals of the workshop. * '''Wednesday 23 June''' - workshop starts at 11:00 (coffee at 10:30). evening: reception and workshop's dinner in the Churchill college * '''Thursday 24 June''' * '''Friday 25 June''' - workshop ends in early afternoon (15:00) a86a8edf9a4265ad4eec4106375480960337ed68 563 562 2010-05-25T13:25:12Z Lukasz 2 wikitext text/x-wiki =Preliminary agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion period. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''It is very likely we will record all presentations in order to make them available through this website. We might also be able to stream the talks live. Details soon.''''' * '''Wednesday 23 June''' - workshop starts at 11:00 (coffee at 10:30). evening: reception and workshop's dinner in the Churchill college * '''Thursday 24 June''' * '''Friday 25 June''' - workshop ends in early afternoon (15:00) 5822b22c82062251e250a08755446b8fa93cbef9 567 563 2010-06-01T13:41:07Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''It is very likely we will record all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We might also be able to stream the talks live. Details soon.''''' {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status<br/> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer<br/> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Posters | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> optional BBQ at the IoA (weather permiting) </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | VOEvent | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Guy Rixon?? |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Walton?? |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 8741ac4fd1e58ca06dd6e43b5c86d301d643871c 583 567 2010-06-09T15:32:33Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''It is very likely we will record all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We might also be able to stream the talks live. Details soon.''''' {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status<br/> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer<br/> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Posters | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | VOEvent | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Guy Rixon?? |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Walton?? |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} cc0f8aa49051e9c4082d84e07c1aa9e213656430 584 583 2010-06-09T16:27:13Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''It is very likely we will record all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We might also be able to stream the talks live. Details soon.''''' {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Walton?? |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} bde96befda23886ffde68c72bbbbf99262d6d80f 585 584 2010-06-09T16:28:15Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''It is very likely we will record all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We might also be able to stream the talks live. Details soon.''''' {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 7cb866089e5379faecc235c77293bcca7cbf7890 589 585 2010-06-15T12:43:21Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How GBOG can help the Gaia ommunity organize itself for multi-site large observational efforts. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Elena Pancino |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alerts distributions possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 217f7dcc9d0c3f7fbf781eeaeaec907ba3d4000f 0 105 565 469 2010-06-01T12:14:57Z Lukasz 2 /* By Air */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus, 30m by train, 1h by bus). Also not too far (approximately 1h 30m by bus, 1h by car) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (buses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are available on-line. It may be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. Taxi from/to Stansted Airport costs about 50 GBP and it takes about 30mins. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 89ef28608ef5e899bef881e46e9c6174474c9db7 566 565 2010-06-01T12:26:14Z Lukasz 2 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus, 30m by train, 1h by bus). Also not too far (approximately 1h 30m by bus, 1h by car) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (buses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are available on-line. It may be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. Taxi from/to Stansted Airport costs about 50 GBP and it takes about 30mins. The cost of a taxi to/from Luton Airport is approximately 70 GBP. The journey takes about 1h. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30 minutes. The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 6b635f0235b1c806a658604e01395a64c6e65306 568 566 2010-06-02T10:32:49Z Lukasz 2 /* Getting to the Institute of Astronomy */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== The closest and more convenient airport to get to Cambridge is London-Stansted (about 45m by bus, 30m by train, 1h by bus). Also not too far (approximately 1h 30m by bus, 1h by car) is London-Luton airport. Several low-cost air companies fly to London-Stansted or London-Luton airports. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. From both airports [http://www.nationalexpress.com NationalExpress] provides a reasonably good bus service (buses every 45m - 1h from Stansted and every 2h from Luton, depending on the time of the day). Time schedule and prices are available on-line. It may be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. Taxi from/to Stansted Airport costs about 50 GBP and it takes about 30mins. The cost of a taxi to/from Luton Airport is approximately 70 GBP. The journey takes about 1h. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 09f7934a71fc571560f5bcba6737b8a74b5f6b24 569 568 2010-06-03T13:13:09Z Lukasz 2 /* By Air */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website]. == London Stansted airport == It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. == London Luton airport == Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP. There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. == London Heathrow airport == London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 1ceeafbec48d924d29ac2e55d2d8ae1b337d544c 570 569 2010-06-03T13:13:51Z Lukasz 2 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website]. === London Stansted airport === It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. === London Luton airport === Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP. There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. === London Heathrow airport === London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 18715eccdec2ed30b2d0432559d649223c895aed 571 570 2010-06-03T13:14:20Z Lukasz 2 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website]. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP. There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. c436846fcb9f9189e3b61f5b9d7f982638b17282 572 571 2010-06-03T13:15:05Z Lukasz 2 /* By Air */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP. A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP. There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 5c78e0bf1b8b098da7696e3030d0b65d88d93571 573 572 2010-06-03T15:04:45Z Lukasz 2 /* Travel */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 079b8a0d7ec01fef57cc8dd86379289f498e3893 587 573 2010-06-15T09:53:22Z Sth 6 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Information for Guests: [[File:130410InfoforGuests.pdf]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 0662750a84c09ce33a3bd32f5948772867ea0c12 588 587 2010-06-15T09:59:00Z Sth 6 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 079b8a0d7ec01fef57cc8dd86379289f498e3893 590 588 2010-06-15T12:50:33Z Sth 6 /* By Air */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact Judith Moss by email if you would like us to make a reservation for you. Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 3185c82b2a80995cd49b4a62f7b5b2243b0a9428 591 590 2010-06-15T12:53:46Z Sth 6 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. f3e7c2448c7c79bc78f1876db5bd4a2223bbe72f 592 591 2010-06-15T12:57:34Z Sth 6 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://www.multimap.com/maps/?hloc=GB|Churchill%20College,%20Cambridge#map=52.21423,0.10446|16|4&bd=useful_information&loc=GB:52.21422:0.10446:17|Storeys%20Way,%20Cambridge|Storey%27s%20Way,%20CAMBRIDGE,%20CB3 Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 31637f264c98ca2d34b435345a477b70992ad6bd 593 592 2010-06-15T12:59:51Z Sth 6 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 3b22b1a47a4d7e63414ea81a46544e854ce348a2 595 593 2010-06-15T13:27:46Z Sth 6 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:GAIA-info-reverse.jpg| 250px | right]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 99bf0978b9ed0bacc90a3972bd86b7c4d7bb9065 597 595 2010-06-15T13:33:56Z Sth 6 /* Accommodation */ wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 1c9f8a3a8dabb713e83a913ef02c14b5cdbdcac6 600 597 2010-06-19T12:00:48Z Sth 6 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] [[Media:130410InfoforGuests.pdf Information on the rooms]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 3b1a5ce2d57a861187c4240b2b286ce9ba07a5e2 6 116 578 2010-06-04T10:41:57Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 117 586 2010-06-15T09:48:09Z Sth 6 Information for guests of Churchill College (2 pages) wikitext text/x-wiki Information for guests of Churchill College (2 pages) 0db9f79293c623be3bab9090f8f9f1c5c6232c08 6 118 594 2010-06-15T13:25:13Z Sth 6 Map of the Ioa and Churchill wikitext text/x-wiki Map of the Ioa and Churchill 6daa13ed14a603a3d9377da1d0bd6de4aecc4053 6 119 596 2010-06-15T13:33:01Z Sth 6 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 105 601 600 2010-06-19T12:02:32Z Sth 6 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] [[Media:130410InfoforGuests.pdf | Information on the rooms]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 48a30e67e865d3a8975b73488db471400b1c0704 602 601 2010-06-19T12:03:03Z Sth 6 wikitext text/x-wiki =Logistics= == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] [[Media:130410InfoforGuests.pdf | Information on the rooms and the college]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 60 GBP per night, double is 75 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 05fa20a5bd2e9470d80ca519347e11bb2404cfc1 0 106 603 589 2010-06-21T09:50:48Z Sth 6 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | TBA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 33622fb5dfd147198b3dc5292fd68cd3b182f858 604 603 2010-06-21T09:58:57Z Sth 6 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Sarah Roberts |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | TBA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} b05fb32a4ee7aaaf2ae6aee681d160eeef8a1230 605 604 2010-06-21T11:03:31Z Sth 6 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | TBA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} d35eb8b71686af945da0aee8b111a9b24ed87cf7 606 605 2010-06-21T11:22:07Z Sth 6 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | NAW/LW/STH/FvL/GG |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 5e22662bcdd9e4f8cfc1b2803d284b560485ef6f 607 606 2010-06-21T11:22:38Z Sth 6 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} ff29d2377b6883a4fd319f5f9055f6b2d8dab62a 608 607 2010-06-21T11:23:27Z Sth 6 wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 18:30(TBC) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 7c8fcca7e014dd3db3ba3045c9b2f2404beae362 609 608 2010-06-21T11:24:39Z Sth 6 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. '''''We will be recording all presentations in order to make them available through this website. Please contact us if you strongly object to being recorded! We will also attempt to stream the talks live. Details soon.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 5d19dca4a574f08e717ab5cee3d023aa53faa0cd 611 609 2010-06-21T15:55:12Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= '''This agenda is still in its draft form and it still might change. Please contact us if you have any comments.''' The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 560fc831c129b611d4e956c22b0b1e1123da8e05 612 611 2010-06-21T15:55:53Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 8906e7ae3c48615009afdb05671cb81a4702a999 615 612 2010-06-22T10:29:59Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> == Abstract book == Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. Please contact us if you wish to amend your abstract. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 4af5cb270145891793b9b103d7099701f12bf32c 617 615 2010-06-22T10:32:43Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. Please contact us if you wish to amend your abstract. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 5774ec24173fc9c312f39948efecc70c19162a57 626 617 2010-06-25T11:18:52Z Lukasz 2 /* Abstract book */ wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. Please contact us if you wish to amend your abstract. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome and update on GREAT | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient and Supernovae searches with PS1 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High energy transients | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Explosive Transient Detection in the Era of Synoptic Sky Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Palomar Transient Factory | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | PTF - The reduction, subtraction, detection, and classification pipelines + some results | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Real-time Transient classification, follow-up and the way forward | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia in the context of low-redshift transient surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The PTF core-collapse supernova key project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Supernova monitor programs | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | GRB science with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia Microlensing Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Microlensing live and in colour | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Accretion-driven transients in the Galaxy | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The galactic population of cataclysmic variables. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Irregular variability during early stellar evolution: what can we learn about the circumstellar material? | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach/Citizen's Science potential of GAIA Science Alert System. | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ground Based Optical Tracking of Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} d67fbfda69b2addf43bd027018a72d4d92856251 627 626 2010-06-25T11:28:12Z Lukasz 2 /* Abstract book */ wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results} | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} e2a035b05a9d53bf3b47a75cc1a7dd015ab4caa1 628 627 2010-06-25T11:29:43Z Lukasz 2 /* Abstract book */ wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Optical transients detected by the Wide Angle Search for Planets (WASP) | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Transient Astronomy with the Liverpool Telescope: Software, Systems and Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The eSTAR Project | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 9bf82eac971889c32f2515e3be890485de6ec049 629 628 2010-06-26T11:25:14Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Discussion - towards the Road Map''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 6cf6f618a52ce689542aa3664ea29f65efb64c1c 630 629 2010-06-26T11:28:54Z Lukasz 2 /* Abstract book */ wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Concluding summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} db1fb3d31173fca1f51a36613af0fdc7546b2dd0 631 630 2010-06-26T11:40:29Z Lukasz 2 /* Abstract book */ wikitext text/x-wiki =Workshop's agenda= The workshop will be structured around invited science presentations and contribution talks, concluding with a discussion periods. We anticipate stimulating significant discussion and tackling the goals of the workshop. All presentations will be recorded and will be published on this website during or soon after the workshop. <big><span style="color:red">!!!</span></big> We would kindly ask and advise you to [mailto:gsaw2010@ast.cam.ac.uk email us] your presentation as a pdf file BEFORE the meeting. We'll keep it as a back-up option in case of any potential technical problems (e.g. broken laptop). AFTER/during the meeting we would like to get the most up-to-date version of you presentation to make it available on this website. <big><span style="color:red">!!!</span></big> ==== Live streaming ==== '''''The presentation will be also streamed live. Please email [mailto:wyrzykow@ast.cam.ac.uk Lukasz Wyrzykowski] if you want to view it.''''' ==== Abstract book ==== Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 0a2b43bbfc54845a501661d4507ea87661b6a08d 632 631 2010-06-26T11:42:06Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | The Gaia mission: a primer | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} acebbb5e71e91e7aaa093f8cc1d15d83106a36c6 633 632 2010-06-30T19:39:24Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | R Coronae Borealis variability and Galactic distribution | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 58299ceed1ba870a9ceac2ec78f7a77b7c5d59c0 634 633 2010-07-01T11:12:24Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Workshop photo | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 4217914b394a1fc27fd4d3ac7c2905adfea5f967 641 634 2010-07-02T08:05:47Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} 0c56f22a684fa72083b25b29b336a98102eedcb8 642 641 2010-07-02T08:06:48Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up opportunities with robotic telescopes | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} d0361f60ab040b2b523a89678033805c444b203f 645 642 2010-07-13T11:09:50Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] 18b379fa8966096b680569d14290573e575fa376 646 645 2010-07-13T11:28:38Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] 333ad49c8b6990a651bdd5f4fa16f60359141f2e 647 646 2010-07-13T11:31:03Z Lukasz 2 /* Workshop's agenda */ wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mignard-MissionPrimer.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia and variable stars ; Ground based follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] 247a15cda33f8e61e21119a6efeb53b1a208ef4b 648 647 2010-07-14T12:59:01Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mignard-MissionPrimer.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Eyer-GSAW.pdf Gaia and variable stars ; Ground based follow-up] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] c7c362b5aa5757c277e22fc655bf6bb62dda1fd3 649 648 2010-07-14T20:22:26Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mignard-MissionPrimer.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/LW-STH-ScienceAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanga-Asteroids.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Smartt-Panstarrs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/OBrien-HighEnergyTransients.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wozniak-Raptor.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ofek-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Poznanski-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wheatley-Wasp.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mahabal-ReadTime.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Sullivan-GaiaInContext.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/GalYam-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Turatto-Supernovae.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Clark-MassiveStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System.] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Eyer-GSAW.pdf Gaia and variable stars ; Ground based follow-up] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] d02015c1d80718b7506192fd4a9a771bbea5a9f7 650 649 2010-07-14T20:31:51Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also recorded and will be published on this website soon. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome address [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Kennicut-Welcome.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rob Kennicut |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mignard-MissionPrimer.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/LW-STH-ScienceAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanga-Asteroids.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Smartt-Panstarrs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/OBrien-HighEnergyTransients.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wozniak-Raptor.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ofek-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Poznanski-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wheatley-Wasp.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mahabal-ReadTime.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/QA-Surveys.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Sullivan-GaiaInContext.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/GalYam-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Turatto-Supernovae.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Clark-MassiveStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanvir-GRBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Levan-GRBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Gould-Microlensing.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Dominik-Microlensing.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Steeghs-Acretion.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Gaensicke-CVs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Kospal-Irregular.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tisserand-RCBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/QA-Science.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ferlet-HandsOnUniverse.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mankiewicz-Outreach.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Altmann-GBOT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Eyer-GSAW.pdf Gaia and variable stars ; Ground based follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Eyer-VariableStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Hudec-CVsSpectra.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Seabroke-RVSAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Lewis-Followup.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Steele-Liverpool.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Naylor-eStar.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/ClosingDiscussion-Summary.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] 49341a34eafdc77c009b77115ee65bcf14d967f2 0 112 610 599 2010-06-21T15:51:18Z Sth 6 wikitext text/x-wiki # Prof. Paul O'Brien, University of Leicester, UK # Dr Timo Prusti, ESA # Prof. Stephen Smartt, Queen's University Belfast, UK # Dr Yael Naze, University of Liege, Belgium # Dr Ashish Mahabal, Caltech, US # Prof. Andy Gould, Ohio State University, US # Dr Przemek Wozniak, Los Alamos, US # Dr Mark Sullivan, Oxford, UK # Dr Laurent Eyer, Geneva, Switzerland # Dr Martin Dominik, St.Andrews, UK # Dr Massimo Turatto, Catania, Italy # Dr David Bersier, Liverpool, UK # Dr Ross Burgon, Open University, UK # Prof. Lech Mankiewicz, PAN Warsaw, Poland # Mr Marcin Wardak, Warsaw, Poland # Dr Dovi Poznanski, Berkeley, US # Dr Paolo Tanga, Nice, France # Dr Avishay Gal-Yam, Weizmann, Israel # Prof. Iain Steele, Liverpool, UK # Dr Martin Altmann, Heidelberg, Germany # Prof. Michel Dennefeld, Paris, France # Dr Eran Ofek, Caltech, US # Dr Danny Steeghs, Warwick, UK # Dr Pavel Koubsky, Ondrejov, Czech Republic # Dr Peter Wheatley, Warwick, UK # Dr Giuseppe Altavilla, Bologna, Italy # Dr Damien Ségransan, University of Geneva, Switzerland # Dr Rene Hudec, Ondrejov, Czech Republic # Mr Mark ter Linden, ESAC, Spain # Dr Sarah Roberts, Cardiff, UK # Dr Patricio F. Ortiz, Leicester, UK # Prof Nial Tanvir, Leicester, UK # Dr George Seabroke, UCL, UK # Dr Tisserand Patrick, Mount Stromlo Observatory, Australia # Dr Boris Gaensicke, Warwick, UK # Dr Andreja Gomboc, Ljubljana, Slovenia # Dr Agnes Kospal, Leiden, The Netherlands # Dr Andrew Levan, Warwick, UK # Dr Ludmila S. Nazarova, Moscow, Russia # Dr Jenny Richardson, Cambridge, UK # Mr Kamil Zloczewski, Warsaw, Poland # Prof. Don Pollacco, Belfast, UK # Prof. Gerry Gilmore, Cambridge, UK # Dr Nick Walton, Cambridge, UK # Prof. Wyn Evans, Cambridge, UK # Dr Simon Clark, Open University, UK # Dr Roger Ferlet, IAP, Paris, France # Dr Francois Mignard, OCA, Nice, France # Dr Lukasz Wyrzykowski, IoA, UK # Dr Sergey Koposov, IoA, UK # Dr Simon Hodgkin, IoA, UK # Dr Nami Mowlavi, Geneva, Switzerland # Professor Tim Naylor, Exeter, UK # Fraser Lewis, Cardiff, UK d21fd2c6d1e22c66d7977558e9326685e097d1db 0 100 613 549 2010-06-22T08:06:14Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:registration|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 70ea95ba323b666913c3b4fad0a6254d15f4691a 614 613 2010-06-22T08:06:58Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Important Dates === * First announcement: '''1st March 2010''' * Registration open: '''1st March 2010''' * Registration closes: '''30 April 2010''' * Support funding allocated: '''10 May 2010''' * Invitations allocated: '''10 May 2010''' * Accommodation and dinner payments: '''20 May 2010''' 901501a4fe2829cb22c368a83c5ee16075fb81f1 621 614 2010-06-24T14:22:47Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo.jpg|thumb|600px]] 1f98aa9d1f602ba8986db16e0fd66962b41abc9f 625 621 2010-06-24T14:35:16Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo.jpg|600px]] a5036a66f3be5cb320a823e0f0d7868fd382b1a7 636 625 2010-07-02T08:00:50Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo.jpg]] d96271fd23552121a318da4122bfc6f0ca8e9df5 637 636 2010-07-02T08:02:55Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] 38e10320a127bc595e20fbdb425887c88dfc5422 639 637 2010-07-02T08:04:29Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] High-resolution version is [[Media:GaiaScienceAlertsWorkshop2010photo.jpg here]]. c7ca2ec8ab8f188bf64136f2af3b25de194822a5 640 639 2010-07-02T08:04:45Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop will take place in Cambridge on 23-25 June 2010 and is supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] High-resolution version is [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|here]]. 1318574cc31208a2364b2c998c9a5ba52acadf96 6 120 616 2010-06-22T10:30:32Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 618 616 2010-06-23T07:19:52Z Lukasz 2 uploaded a new version of "[[File:Gsaw-abstract book.pdf]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 619 618 2010-06-23T07:23:25Z Lukasz 2 uploaded a new version of "[[File:Gsaw-abstract book.pdf]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 620 619 2010-06-23T07:24:21Z Lukasz 2 uploaded a new version of "[[File:Gsaw-abstract book.pdf]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 643 620 2010-07-06T14:23:58Z Lukasz 2 uploaded a new version of "[[File:Gsaw-abstract book.pdf]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 121 622 2010-06-24T14:26:41Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 623 622 2010-06-24T14:28:11Z Lukasz 2 uploaded a new version of "[[File:GaiaScienceAlertsWorkshop2010photo.jpg]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 624 623 2010-06-24T14:30:45Z Lukasz 2 uploaded a new version of "[[File:GaiaScienceAlertsWorkshop2010photo.jpg]]" wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 4 122 635 2010-07-01T15:35:03Z Lukasz 2 Created page with 'Gaia Science Alerts Working Group is an informal group of researchers willing to exploit the near-real-time alerts from the Gaia satellite. The group is closely linked with DPAC ...' wikitext text/x-wiki Gaia Science Alerts Working Group is an informal group of researchers willing to exploit the near-real-time alerts from the Gaia satellite. The group is closely linked with DPAC (Data Processing and Analysis Consortium) Photometry Unit (CU5), which is responsible for delivery of the alerts after the launch of the mission in 2012. The group is also immediately connected with the Science Alerts WG of [http://www.ast.cam.ac.uk/GREAT/index.html GREAT] network, supported by European Commission. Anyone interested in Gaia Science Alerts is invited to contribute to the group. Please contact the administrator if you want to obtain the edit password. 366d675842f7dc8970ff742ef098b3a6222c6d74 6 123 638 2010-07-02T08:03:32Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 124 644 2010-07-12T10:11:33Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 125 651 2010-09-09T09:14:41Z Gaia 3 For testing upload wikitext text/x-wiki For testing upload 8b627520b14f9d718c0183b4a6aa75666e0ed194 6 126 652 2010-09-09T10:09:21Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 100 653 640 2010-10-22T12:01:13Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop took place in Cambridge on 23-25 June 2010 and was supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] High-resolution version is [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|here]]. 2ccf83ca37b155fa3dcbff9189a55857cb576b66 656 653 2010-10-22T14:56:57Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop took place in Cambridge on 23-25 June 2010 and was supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] ---- <big>Post-workshop White Book is available [[Media:Postgsaw_wb.pdf|here]]</big> ---- * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] High-resolution version is [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|here]]. 1fff595e19f341859674475be3e286b53c05df13 657 656 2010-10-22T14:58:04Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop took place in Cambridge on 23-25 June 2010 and was supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] ---- <center> <big>Post-workshop White Book is available [[Media:Postgsaw_wb.pdf|here]]</big></center> ---- * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] High-resolution version is [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|here]]. f145dabd65ad5d9e662689977a6bc9eb77ff5306 664 657 2010-11-09T14:40:42Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop took place in Cambridge on 23-25 June 2010 and was supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] ---- <center> <big>Post-workshop White Book is available [[Media:Postgsaw_wb.pdf|here]]</big></center> ---- * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo_small.jpg]] High-resolution version is [[File:GaiaScienceAlertsWorkshop2010photo.jpg|here]]. 552debec6fe3618222eb9459c7d958b9885bd4e3 665 664 2010-11-09T14:42:33Z Lukasz 2 /* Workshop photo */ wikitext text/x-wiki == Welcome! == [[File:great-esf-logo.png|right|200px]] Gaia Science Alerts Workshop took place in Cambridge on 23-25 June 2010 and was supported by the ESF grant [http://www.ast.cam.ac.uk/GREAT/ GREAT] ---- <center> <big>Post-workshop White Book is available [[Media:Postgsaw_wb.pdf|here]]</big></center> ---- * [[workshop2010:rationale|Rationale]] * [[workshop2010:agenda|Agenda]] * [[workshop2010:participants|Participants]] * [[workshop2010:logistics|Logistic information]] * [[workshop2010:poster|Workshop's poster for download]] [[File:GAIA-2010web-poster.jpg|right|200px]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Vasily Belokurov * Wyn Evans * Gerry Gilmore * Floor van Leeuven * Sergey Koposov * Nick Walton If you wish to contact the organizing committee, please email ''gsaw2010woc@ast.cam.ac.uk''. ---- === Workshop photo === [[File:GaiaScienceAlertsWorkshop2010photo.jpg|600px]] 9a961c2daa0a9380581a0d07414fd76f184d2e9d 0 106 654 650 2010-10-22T12:03:33Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also video recorded and are available in AVI format. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome address [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Kennicut-Welcome.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rob Kennicut |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mignard-MissionPrimer.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/LW-STH-ScienceAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanga-Asteroids.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Smartt-Panstarrs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/OBrien-HighEnergyTransients.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wozniak-Raptor.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ofek-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Poznanski-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wheatley-Wasp.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mahabal-ReadTime.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/QA-Surveys.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Sullivan-GaiaInContext.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/GalYam-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Turatto-Supernovae.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Clark-MassiveStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanvir-GRBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Levan-GRBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Gould-Microlensing.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Dominik-Microlensing.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Steeghs-Acretion.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Gaensicke-CVs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Kospal-Irregular.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tisserand-RCBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/QA-Science.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ferlet-HandsOnUniverse.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mankiewicz-Outreach.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Altmann-GBOT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Eyer-GSAW.pdf Gaia and variable stars ; Ground based follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Eyer-VariableStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Hudec-CVsSpectra.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Seabroke-RVSAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Lewis-Followup.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Steele-Liverpool.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Naylor-eStar.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/ClosingDiscussion-Summary.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] 38e747305ec609ada5b8f6f0ea285d896738dbc9 6 127 655 2010-10-22T14:53:38Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 128 658 2010-10-28T10:45:35Z Lukasz 2 Created page with '[http://uk.arxiv.org/abs/1010.5695 Sturm et al.(2010)] cross-matched an X-ray outburst source with a Be-type star exhibiting optical outbursts of 0.5 mag every around 1000 days. ...' wikitext text/x-wiki [http://uk.arxiv.org/abs/1010.5695 Sturm et al.(2010)] cross-matched an X-ray outburst source with a Be-type star exhibiting optical outbursts of 0.5 mag every around 1000 days. [[File:XrayBin-Sturm2010.png]] d1a2a4e451cb2ff5d8f0f904824ef0611ade04ae 660 658 2010-10-28T10:46:40Z Lukasz 2 wikitext text/x-wiki [http://uk.arxiv.org/abs/1010.5695 Sturm et al.(2010)] cross-matched an X-ray outburst source with a Be-type star exhibiting optical outbursts of 0.5 mag every around 1000 days. [[File:XrayBin-Sturm2010.png]] c30c0bbeb452ee6255a1a1f961bd49d90cddf937 661 660 2010-10-28T10:47:19Z Lukasz 2 wikitext text/x-wiki [http://uk.arxiv.org/abs/1010.5695 Sturm et al.(2010)] cross-matched an X-ray outburst source with a Be-type star exhibiting optical outbursts of 0.5 mag every around 1000 days. [[File:XrayBin-Sturm2010.png|400px]] d159f4f7ad061df015c3d61755c2fdeeabfdce46 6 129 659 2010-10-28T10:46:11Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 42 662 228 2010-10-28T13:51:35Z Lukasz 2 wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- === Detection efficiency for Gaia === Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge. Assuming mean time-scale of 30 days and mean detection efficiency for events before the peak of 30%, it means about a 1000 events towards the Bulge should be detected by Gaia. This number, however, might be affected by crowding effects in the Bulge. On the other hand, the satellite is planned to be slowed down a bit to observe Baade's Window (towards the Bulge) more frequently, what can increase the efficiency of detection. Over entire sky there is something like 750 events expected to happen during the mission. If the mean time-scale is about 15 days, the mean efficiency is about 20%, thus there should be additional 150 events detected all over the sky before they reach the peak brightness. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days. For detections before the peak.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days. For detections before the peak.]] ---- === Astrometry of microlensing events === [http://adsabs.harvard.edu/abs/2002MNRAS.331..649B Belokurov&Evans 2002] a514c7d642cc95cc783b27536af321a5239d2881 663 662 2010-10-28T13:52:03Z Lukasz 2 wikitext text/x-wiki === Standard events === Amplitude: can be many magnitudes, in range 0.1-10 mag. Time-scale: is defined as Einstein Ring crossing time and is close to FWHM of the bell-like light curve of the event. The light curves are usually symmetric with slow rise and slow decline. In case of high magnification, the rise in magnitude speeds up closer to the peak. Sources: can be located anywhere, however, the further source, the higher chance of it being microlensed. [[File:example_standard_event.png|300px]] === Exotic events === It is believed, around 10% of all events (at least towards the bulge) exhibit some kind of anomalous behaviour. In most cases it due to binary companion either to the source or the lens. The light curves are then usually asymmetric, with high amplification regions and sharp rises in magnitude in case of binary lenses. [[File:example_binary_lens.png|400px]] Figure from [http://ukads.nottingham.ac.uk/abs/2004AcA....54..103J Jaroszynski et al. 2004]. ---- == OGLE's EWS == OGLE Early Warning System ([http://ogle.astrouw.edu.pl/ogle3/ews/ews.html EWS]) is detecting in real-time about 600 events per year towards the Galactic bulge. [[File:plot_ews_te_ampl.png|300px]] [[File:plot_ews_te_baselinemag.png|300px]] Distribution of time scales corrected for detection efficiency for OGLE-III Bulge events. [[File:plot_ulensing_distrib_tE.png|400px]] ---- == All-sky events == 99% of events are currently being detected towards the Galactic Centre, due to its largest optical depth. There is couple of events reported towards the Magellanic Cloud. Serendipitous detection of a microlensing event located not in the crowded field: [http://ukads.nottingham.ac.uk/abs/2008ApJ...677.1268G Gaudi et al. 2008] GSC 3656-1328 [[File:GSC3656-1328.png|300px|Light curve of GSC 3656-1328 microlensing event]] [[File:Han-tau.png|300px|Probability of all-sky microlensing (optical depth) in units of 10-8 for sources down to V=18 mag.]] [[File:plot_prob_microlensing.png|300px|Estimated probability of all-sky microlensing, including lensing in the Bulge. Units 1e-8.]] ---- === Detection efficiency for Gaia === Over 5 years of operation of Gaia, there should be around 3000 microlensing events occurring in the Bulge. Assuming mean time-scale of 30 days and mean detection efficiency for events before the peak of 30%, it means about a 1000 events towards the Bulge should be detected by Gaia. This number, however, might be affected by crowding effects in the Bulge. On the other hand, the satellite is planned to be slowed down a bit to observe Baade's Window (towards the Bulge) more frequently, what can increase the efficiency of detection. Over entire sky there is something like 750 events expected to happen during the mission. If the mean time-scale is about 15 days, the mean efficiency is about 20%, thus there should be additional 150 events detected all over the sky before they reach the peak brightness. [[File:plot_eff_te15.0000_riseonly.png|left|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 15 days. For detections before the peak.]] [[File:plot_eff_te100.000_riseonly.png|right|thumb|300px|Microlensing events detection efficiency by Gaia for events with time-scale of 100 days. For detections before the peak.]] ---- == Astrometry of microlensing events == [http://adsabs.harvard.edu/abs/2002MNRAS.331..649B Belokurov&Evans 2002] 406a31ad936408be8544f45e1e62cb5cfd8b14c8 0 11 666 508 2010-11-12T10:55:32Z Lukasz 2 major update of the description. wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with the dedicated network of follow-up telescopes operating in the ''Target of Opportunity'' (ToO) mode. The verification observations should be carried both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. Verification Phase should reveal all necessary adjustments which has to be done to the detection and classification algorithms to assure the best and the most robust performance later on. Verification Phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects. Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for early start of the alerting pipeline. In principle, some pre-launch preparations could take place in the areas of very dense Gaia observations. It includes gathering all useful information about the objects in these regions both from existing catalogues and with new observations. The information includes, among the others, variability classification and spectral type classification. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with Gaia alerts stream when they become fully public. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Loiano || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Bologna, Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} 24f8f71f459922ac0228408acf41bb7ae9205e8e 667 666 2010-11-12T13:41:41Z Sth 6 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Loiano || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Bologna, Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} 1a17fa2df521440dcf8a66ee20d25582415b0cda 673 667 2010-11-19T17:17:52Z Lukasz 2 /* Preliminary list of telescopes and people involved */ wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Loiano || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Bologna, Italy |- |Padova || Gisella Clementini || ? Padova, Italy |- |Catania || Gisella Clementini || 80cm Ritchey-Chretien, f/8, Serra la Nave, Catania, Sicily |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 40ab55ce005c546f24b74feab776f85866a887fc 674 673 2010-11-19T17:39:01Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || 80cm Ritchey-Chretien, f/8, Serra la Nave, Catania, Sicily |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 46c18ec6694b27261ed583349ab2494438644488 675 674 2010-11-29T11:42:19Z Lukasz 2 /* Preliminary list of telescopes and people involved */ wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Chretien (APT2), Serra la Nave, Catania, Sicily |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 2cce98529b2c92dcc9984315c996b24082dd2b09 0 40 668 348 2010-11-16T10:01:52Z Lukasz 2 wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. 9084b6cec0fc40fb42724cc9d3347dbbc0078124 669 668 2010-11-16T15:51:55Z Lukasz 2 /* Supernovae type II */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. 58ad6f31ec43991f37673758e177acb0d0cff750 0 8 670 505 2010-11-16T15:58:20Z Lukasz 2 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:FUOri | FU Orionis-type eruptive stars]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:Supernovae | Supernovae]] * [[Triggers:TTau | T Tauri type pre-main sequence stars]] * [[Triggers:XBs | X-ray binaries (XBs)]] * [[Triggers:Other | Other rare transients]] * [[Triggers:Theoretical | Exotic/theoretical events]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] eba42c1573b7004c60d89c80ed590b85aae726b6 0 130 671 2010-11-16T16:01:07Z Lukasz 2 Created page with '* Tidal disruption events [http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full_html/2009/08/aa11479-08/aa11479-08.html] * Lensing b...' wikitext text/x-wiki * Tidal disruption events [http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full_html/2009/08/aa11479-08/aa11479-08.html] * Lensing by cosmic strings * Optical counterparts to gravitational wave events [https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=1756&version=0] 3bada72ff0f9d6143142066c094b7317fe10b08d 0 1 672 370 2010-11-16T16:04:47Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''[[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]]'''</center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- faac47e70adc2a9b53b9a762537d1fb349ee7dda 676 672 2010-12-14T13:22:56Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>Workshop 2011 - Gaia alerts verification and follow-up</Big> June 2011, Cambridge ''details soon'' Please contact [[user:lukasz|L. Wyrzykowski]] if you would like to attend it. ---- '''[[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]]'''</center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 750cba7eebc8a08389897e9a7e20823e5b41c732 677 676 2010-12-14T13:23:35Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>Workshop 2011 - Gaia alerts verification and follow-up</Big> June 2011, Cambridge ''details soon'' Please contact [[user:lukasz|L. Wyrzykowski]] if you would like to attend it. </center> ---- <center> [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 1a569251cfefd6cceb25f9e8b018b71dc86b49d1 678 677 2010-12-22T16:21:53Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>Workshop 2011 - Gaia alerts verification and follow-up</Big> June 2011, Cambridge ''details soon [[Workshop2011:main|here]]'' Please contact [[user:lukasz|L. Wyrzykowski]] if you would like to attend it. </center> ---- <center> [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 0bf4c21e65083fa5258a04b4d5f24cd2eef2c49c 688 678 2011-01-31T15:42:26Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>Workshop 2011 - Gaia alerts verification and follow-up</Big> June 2011, Cambridge ''details [[Workshop2011:main|here]]'' </center> ---- <center> [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 794375bf84cc57b58ab7107aafb43144aa2d4477 690 688 2011-01-31T15:43:11Z Gsawgwikiadmin 1 /* Welcome to the web site of the Gaia Science Alerts Working Group! */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>Workshop 2011 - Gaia alerts verification and follow-up</Big> 29th June - 1st July 2011, Cambridge ''details [[Workshop2011:main|here]]'' </center> ---- <center> [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- c2d69a4889baa59024150fd8de929fc367242728 0 131 679 2010-12-22T16:25:20Z Lukasz 2 Created page with 'The first workshop on Gaia Science Alerts, was held in June 2010 in Cambridge. We introduced the Science Alerts concept to a broad group of scientists from the international astr...' wikitext text/x-wiki The first workshop on Gaia Science Alerts, was held in June 2010 in Cambridge. We introduced the Science Alerts concept to a broad group of scientists from the international astronomical community. During the workshop key areas of interest were defined, and potential Gaia contributions to these fields were discussed in detail. The Gaia Science Alerts stream will be the first Gaia data released to the community, so it is extremely important to produce reliable and robust alerts. To ensure that the released alerts are accurately classified, low in contaminants and contain interesting transient events, the complex data processing pipeline has to be thoroughly tested. The first alerts will need to be verified with an extensive programme of dedicated follow-up observations. These comprise: * imaging to confirm the presence and brightness of an alerting source, * continuous photometric monitoring to obtain a detailed light-curve to help fine-tune the classification * high/intermediate resolution spectroscopy to investigate the real nature of an event. ---- The verification programme is scheduled to take place in the first three months of operation of the Gaia Science Alert system. To classify as many alerts as possible requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. A meeting scheduled for next summer is the best way to achieve our primary goals: * Familiarisation of potential observers and research groups with Gaia and its alerting system, and the specific requirements of verification. * A plan of the detailed scope of the alerts verification phase, including how long it should last * Selection of likely telescopes and instruments * Identification of key people who will assist with verification * Confirmation of the scientific requirementss for the follow-up of Gaia alerts, e.g. in the area of supernovae or cataclysmic variables * Discussion of technical issues related with alert dissemination and follow-up feedback ---- During the interactive workshop we plan to bring together: * Experts on the Gaia mission, including Gaia Science Alerts * People responsible for telescopes around the globe * Astronomers experienced with observations of transient phenomena * Scientists and experts active in studying transient phenomena * Scientists involved in the distribution of alerts, e.g. from skyalert.org * Individuals interested in the outreach possibilities of Gaia Science Alerts e6cb0548a1fc037985a28ace1d824bee563cd291 683 679 2011-01-31T15:34:57Z Lukasz 2 Replaced content with 'The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011.' wikitext text/x-wiki The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. 3d03c7c14cc2bb386ff2dacb454572378d021be8 686 683 2011-01-31T15:40:20Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:participants|Participants]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven 1044a64d23199bf4e9caea42d1b54263baeff713 687 686 2011-01-31T15:40:59Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:participants|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven b28dd3bafb11b5db25bce712a707a0a6431e5a33 698 687 2011-02-01T15:23:01Z Lukasz 2 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven 8c0b8131b5c5c0a45467c4071726cb9620deb10e 699 698 2011-02-01T15:23:39Z Lukasz 2 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss 5399495bb6dd1fae9bcafc92eba4bdd045f13134 8 3 680 499 2011-01-22T11:32:06Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2011 ** workshop2011:main:Main Workshop Page * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:rationale|Rationale ** workshop2010:agenda|Agenda (archive) ** workshop2010:registration|Registration / Participants ** workshop2010:logistics|Logistics * SEARCH * TOOLBOX 5b68a70ac8715d092bfb62313b8c01d9a983c63c 681 680 2011-01-22T11:32:37Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2011 ** workshop2011:main|Main Workshop Page * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:rationale|Rationale ** workshop2010:agenda|Agenda (archive) ** workshop2010:registration|Registration / Participants ** workshop2010:logistics|Logistics * SEARCH * TOOLBOX bb67efecf3ff1e30f50cdd5b3a3ca6af981f7d11 682 681 2011-01-22T11:33:44Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2011 ** workshop2011:main|Main Workshop Page * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:rationale|Rationale ** workshop2010:agenda|Agenda (archive) ** workshop2010:registration|Registration / Participants ** workshop2010:logistics|Logistics * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX b4c9a2686e38db31b12a83fd58382ecf75db584a 684 682 2011-01-31T15:37:30Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2011 ** workshop2011:main|Main Workshop Page ** workshop2011:rationale|Rationale ** workshop2011:agenda|Agenda ** workshop2011:registration|Registration / Participants ** workshop2011:logistics|Logistics * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 2358bd9762503161121768bb203232c1ab365c69 0 132 685 2011-01-31T15:37:53Z Gsawgwikiadmin 1 Created page with 'The first workshop on Gaia Science Alerts, was held in June 2010 in Cambridge. We introduced the Science Alerts concept to a broad group of scientists from the international astr...' wikitext text/x-wiki The first workshop on Gaia Science Alerts, was held in June 2010 in Cambridge. We introduced the Science Alerts concept to a broad group of scientists from the international astronomical community. During the workshop key areas of interest were defined, and potential Gaia contributions to these fields were discussed in detail. The Gaia Science Alerts stream will be the first Gaia data released to the community, so it is extremely important to produce reliable and robust alerts. To ensure that the released alerts are accurately classified, low in contaminants and contain interesting transient events, the complex data processing pipeline has to be thoroughly tested. The first alerts will need to be verified with an extensive programme of dedicated follow-up observations. These comprise: * imaging to confirm the presence and brightness of an alerting source, * continuous photometric monitoring to obtain a detailed light-curve to help fine-tune the classification * high/intermediate resolution spectroscopy to investigate the real nature of an event. ---- The verification programme is scheduled to take place in the first three months of operation of the Gaia Science Alert system. To classify as many alerts as possible requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. A meeting scheduled for next summer is the best way to achieve our primary goals: * Familiarisation of potential observers and research groups with Gaia and its alerting system, and the specific requirements of verification. * A plan of the detailed scope of the alerts verification phase, including how long it should last * Selection of likely telescopes and instruments * Identification of key people who will assist with verification * Confirmation of the scientific requirementss for the follow-up of Gaia alerts, e.g. in the area of supernovae or cataclysmic variables * Discussion of technical issues related with alert dissemination and follow-up feedback ---- During the interactive workshop we plan to bring together: * Experts on the Gaia mission, including Gaia Science Alerts * People responsible for telescopes around the globe * Astronomers experienced with observations of transient phenomena * Scientists and experts active in studying transient phenomena * Scientists involved in the distribution of alerts, e.g. from skyalert.org * Individuals interested in the outreach possibilities of Gaia Science Alerts e6cb0548a1fc037985a28ace1d824bee563cd291 0 133 689 2011-01-31T15:42:44Z Gsawgwikiadmin 1 Created page with 'Workshop will be limited to 35 participants. Please contact [[user:lukasz|L. Wyrzykowski]] if you would like to attend it.' wikitext text/x-wiki Workshop will be limited to 35 participants. Please contact [[user:lukasz|L. Wyrzykowski]] if you would like to attend it. 8138e3b8b4b7989537bf48384be07da74ae8f9cb 0 134 691 2011-01-31T15:44:42Z Gsawgwikiadmin 1 Created page with ' == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchil...' wikitext text/x-wiki == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] [[Media:130410InfoforGuests.pdf | Information on the rooms and the college]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 63 GBP per night, double is 75 GBP (TBC) per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsaw2010@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 4857a855d3e12ef59e8a990278c621efc87a8e9f 692 691 2011-01-31T15:50:15Z Gsawgwikiadmin 1 wikitext text/x-wiki == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] [[Media:130410InfoforGuests.pdf | Information on the rooms and the college]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 63 GBP per night, double is 75 GBP (TBC) per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 20th of May 2010.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsawg@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 24dce50eb0b4ffec61cb51cf63dee145242bdc96 0 135 693 2011-02-01T13:36:56Z Lukasz 2 Created page with '==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''If you would like to attend the ...' wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''If you would like to attend the workshop, or received an invitation, please fill the form [[Workshop2011:registrationform | here]]''' 7402c68cb42010c525bacf0422a8af868f69e35b 694 693 2011-02-01T13:37:42Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''If you would like to attend the workshop, or received an invitation, please fill the form [[Workshop2011:registrationform | here]]''' ==== Participants ==== 3e2dad0ee805090f903005a83167bf3c0ef8915d 0 136 695 2011-02-01T13:48:57Z Lukasz 2 Created page with '== Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast....' wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=28/06/2011}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=01/07/2011}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 57 GBP per night *twin at 70 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on'' '''''Thursday 30th''''' ''in the college. The estimated cost would be around 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 1fdccd10969d39bc04d8ef84a04e1dbf8290c2d2 696 695 2011-02-01T13:53:27Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer-invitee.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=28/06/2011}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=01/07/2011}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 57 GBP per night *twin at 70 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on'' '''''Thursday 30th''''' ''in the college. The estimated cost would be around 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 6fb8a18a76025661fca94f470567b69d826a4102 697 696 2011-02-01T13:56:27Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=28/06/2011}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=01/07/2011}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 57 GBP per night *twin at 70 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to host a workshop's reception and dinner on'' '''''Thursday 30th''''' ''in the college. The estimated cost would be around 50 GBP.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 63255437ebbfeb791a884c82ef3ef90545c9332a 700 697 2011-02-01T15:24:59Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| |- | Requested from date: | {{#input:type=text|name=accom_from|value=28/06/2011}} | Check-out date: | {{#input:type=text|name=accom_checkout|value=01/07/2011}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 57 GBP per night *twin at 70 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 30th''''' ''in the St.John's Chop House restaurant.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} f1eabd44c9aa909c559dae34b68682bd5fcc1528 0 134 701 692 2011-02-02T13:59:26Z Lukasz 2 wikitext text/x-wiki == Accommodation == The organizers have booked number of rooms in the nearby [http://www.chu.cam.ac.uk/ Churchill College]. [[File:Churchill1.jpg|250px|right]] [[File:Churchill2.jpg|250px|right]] [[File:Screen_shot_2010-06-15_at_14.32.12.png | 250px | right]] [[Media:130410InfoforGuests.pdf | Information on the rooms and the college]] Churchill College: [http://www.churchillconferences.co.uk/media/downloads/Churchill%20plans%20%28for%20web%29.pdf SIte Map] [http://maps.google.co.uk/maps?client=safari&rls=en&q=cb3+0ha&oe=UTF-8&redir_esc=&um=1&ie=UTF-8&hq=&hnear=Cambridge+CB3+0HA&gl=uk&ei=5ngXTMngCYz00gT7opnUCw&sa=X&oi=geocode_result&ct=title&resnum=1&ved=0CBUQ8gEwAA Google Map of the Area] Description of the rooms from the College's website: ''The light, generously proportioned rooms combine the functional needs of a business traveller, including a spacious desk and free broadband internet access, with home comforts such as a hospitality tray and toiletries.'' ''Additional facilities for residents include an on-site laundry, a TV room, an all day bar and cafe (subject to opening hours) and sports facilities including squash and tennis courts and a multi-gym. Sports equipment, irons and hair dryers can all be borrowed from the Porters' Lodge.'' '' Many of the rooms offer views over the inner courtyards or surrounding grounds and gardens.'' ''The rooms we are offering have en-suite toilet and shower and continental breakfast is included in the price. Single room is 58 GBP per night, double is 72 GBP per night.'' '''If you are interested in taking this accommodation please state it on your registration form. Number of rooms is limited. You will be asked to pay for your accommodation in advance before 1st of June 2011.''' Alternatively, check out one of the following websites, which provide an extensive list of hotels and B&B in the Cambridge area: *[http://www.visitcambridge.org/wheretostay.php B&B Visit Cambridge] *[http://www.ukaccommodationindex.com/cambridge.php B&B Cambridge] The workshop is taking place at the Institute of Astronomy on Madingley Road, so the closest options are Canterbury House (B&B), Benson House (Guest House), the [http://www.premierinn.com/pti/hotelInformation.do?hotelId=26708 Premier Inn] (Hotel) or the [http://www.arundelhousehotels.co.uk/ Arundel House Hotel]. == Travel == ===By Air=== You can check various options at [http://www.skyscanner.net this website], mainly for cheap flights. '''A word about taxis''' We recommend pre-arranging taxi bookings with a Cambridge taxi firm, e.g. Panther Taxis +44 1223 715715, or alternatively contact us [mailto:gsawg@ast.cam.ac.uk by email] if you would like us to make a reservation for you (please put the word TAXI in the subject line to help us spot it). Catching a black cab from Heathrow airport could cost you several hundred pounds, at least double the price of a private hire booking. ==== London Stansted airport ==== It is the closest and the most convenient airport to get to Cambridge. Some cheap airlines fly there, e.g. [http://www.ryanair.com RyanAir] or [http://www.easyjet.com EasyJet]. Direct buses to Cambridge are operated by [http://www.nationalexpress.com NationalExpress] and run almost every hour. Journey takes about 1h. It might be better to buy your bus ticket as soon as you know your flight details, but there is also a possibility for buying your ticket at the counter at the airport. By car/taxi it takes about 30-40 minutes. Taxi costs about 50 GBP (+30% between 12 and 5am). A train service is also provided from Stansted Airport to Cambridge. Schedules and prices can be found at [http://www.thetrainline.com http://www.thetrainline.com]. It takes about 30 minutes to/from Cambridge. ==== London Luton airport ==== Several low-cost air companies fly to/from Luton. Among others check [http://www.ryanair.com RyanAir], [http://www.easyjet.com EasyJet] and [http://www4.germanwings.com GermanWings]. There is a regular direct bus service from the airport to Cambridge around every 2h. Journey takes about 1.5h. Check times and prices on the [http://www.nationalexpress.com NationalExpress] website. By car/taxi it takes at least 1h, depending on the traffic. Taxi costs about 70 GBP (+30% between 12 and 5am). There is also a possibility to get to London first and then to Cambridge by train. It takes about 2-2.5h. ==== London Heathrow airport ==== London Heathrow airport is also an option with all major airlines flying there. From/to Cambridge it takes about 2.5-3h by a direct bus ([http://www.nationalexpress.com NationalExpress]) and 1.5h by car. Taxi to/from Heathrow costs around 100 GBP (+30% between 12 and 5am). Another option is to take an underground (Piccadilly Line) to King's Cross (about 1h) and then a train to Cambridge (another 1-1.5h). ==== London Gatwick airport ==== There is a direct bus between Gatwick and Cambridge, but it takes around 4h. Taxi costs about 125 GBP (+30% between 12 and 5am). The easiest option seems to be the Gatwick Express train to/from Victoria Station in London. ==== London City airport ==== This small airport is a convenient alternative. Some major airlines fly there (e.g. BA, LH, Swiss). Taxi to/from Cambridge costs about 80 GBP (+30% between 12 and 5am). Another option is the underground (DLR and other lines) to King's Cross train station and a train to Cambridge. Check [http://www.tfl.gov.uk Transport for London website] for detailed schedules of the underground. ===By Train=== [http://www.eurostar.com Eurostar] offers quite good fares when buying tickets in advance. So if you are coming from Paris or Bruxells (for more destinations please check the website) consider this option as well. Eurostar trains arrive at St. Pancras International, you will need to get to Kings Cross Station (the two stations are within a few hundred meters) to get the train to Cambridge. For time schedules and prices check this website [http://www.thetrainline.com http://www.thetrainline.com]. ===Local transportation=== Both the Cambridge train and bus stations are quite close to the centre of the city. Local busses schedules can be seen on-line at this website [http://www.cambridgeshire.gov.uk/transport/bus_timetables http://www.cambridgeshire.gov.uk/transport/bus_timetables]. ==Getting to the Institute of Astronomy== The following link takes you to the official map prepared by the University of Cambridge (the map is currently set to show in the centre the location of the [http://www.ast.cam.ac.uk Institute of Astronomy] but scrolling and zooming are both possible) : [http://www.cam.ac.uk/map/v3/drawmap.cgi?mp=main;xx=700;yy=240;gf=png link to the map]. There is not direct bus running from the train station to the IoA, therefore we recommend taking a taxi. From the Park Side bus station, or just City Centre, you can take bus no City4. Buy the ticket from the driver to ''Thompson Avenue''. Walk from the City Centre to the IoA takes about 30-45 minutes. From the Churchill College it takes about 10 minutes along Madingley Road (there is also shortcut available through the sports grounds, then enter the "woods" after the college chapel to reach the IoA's Main Library). The University of Cambridge also has a webpage providing some local information for visitors. This can be found at [http://www.cam.ac.uk/cambuniv/visitors this link]. 62b71d9ee7fc38ff6c1be52b759e5f3d0b3fb24c 0 136 702 700 2011-02-02T14:08:35Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- ''' Arrival/departure''' Please provide us with the dates of your arrival/departure to/from Cambridge: {| |- | Arrival: | {{#input:type=text|name=arrival|value=28/06/2011}} | Departure: | {{#input:type=text|name=departure|value=01/07/2011}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College from 28/06 to 01/07 (contact us if you need to book for other dates) | {{#input:type=select|name=accom_churchill| *Please select *yes *no, I'll find accommodation myself}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 58 GBP per night *twin at 72 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 30th''''' ''in the St.John's Chop House restaurant.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 93431d0c333cd775e972f30016d2eb706adf22d4 703 702 2011-02-02T14:09:32Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- ''' Arrival/departure''' Please provide us with the dates of your arrival/departure to/from Cambridge: {| |- | Arrival: | {{#input:type=text|name=arrival|value=28/06/2011}} | Departure: | {{#input:type=text|name=departure|value=01/07/2011}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College from 28/06 to 01/07 (contact us if you need to book for other dates) | {{#input:type=select|name=accom_churchill| |- *Please select *yes *no, I'll find accommodation myself}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 58 GBP per night *twin at 72 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 30th''''' ''in the St.John's Chop House restaurant.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 5ec5df94042ca7f9af8c53342d801c0b40f91a24 6 137 704 2011-02-02T14:56:47Z Lukasz 2 Gilmore's presentation on GBOG and Alerts Verification wikitext text/x-wiki Gilmore's presentation on GBOG and Alerts Verification 4d28dedbfed3004fd1a4ab733120498ba611f7cc 0 135 705 694 2011-02-15T13:51:22Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. <big>The registration closes on '''1st June 2011'''. '''If you would like to attend the workshop please fill the form [[Workshop2011:registrationform | here]].''' </big> ---- ==== List of Participants ==== 6f63f5953eee986b45267272b687d060794e2a9c 711 705 2011-03-08T14:02:00Z Lukasz 2 /* List of Participants */ wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. <big>The registration closes on '''1st June 2011'''. '''If you would like to attend the workshop please fill the form [[Workshop2011:registrationform | here]].''' </big> ---- ==== List of Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Kailash Sahu, STSI, USA # Danny Steeghs, Warwick, UK bf0505cb510942d012e26e67438a242179223267 712 711 2011-03-08T14:02:28Z Lukasz 2 /* List of Participants */ wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. <big>The registration closes on '''1st June 2011'''. '''If you would like to attend the workshop please fill the form [[Workshop2011:registrationform | here]].''' </big> ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Kailash Sahu, STSI, USA # Danny Steeghs, Warwick, UK 420f1cb14ae3e5d125bb0ed61401bcc6e2405bf2 0 132 706 685 2011-02-15T17:21:19Z Lukasz 2 wikitext text/x-wiki The first workshop on Gaia Science Alerts, was held in June 2010 in Cambridge. We introduced the Science Alerts concept to a broad group of scientists from the international astronomical community. During the workshop key areas of interest were defined, and potential Gaia contributions to these fields were discussed in detail. The Gaia Science Alerts stream will be the first Gaia data released to the community, so it is extremely important to produce reliable and robust alerts. To ensure that the released alerts are accurately classified, low in contaminants and contain interesting transient events, the complex data processing pipeline has to be thoroughly tested. The first alerts will need to be verified with an extensive programme of dedicated follow-up observations. These comprise: * imaging to confirm the presence and brightness of an alerting source, * continuous photometric monitoring to obtain a detailed light-curve to help fine-tune the classification * high/intermediate resolution spectroscopy to investigate the real nature of an event. ---- The verification programme is scheduled to take place in the first three months of operation of the Gaia Science Alert system. To classify as many alerts as possible requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. A meeting scheduled for next summer is the best way to achieve our primary goals: * Familiarisation of potential observers and research groups with Gaia and its alerting system, and the specific requirements of verification. * A plan of the detailed scope of the alerts verification phase, including how long it should last * Selection of likely telescopes and instruments * Identification of key people who will assist with verification * Confirmation of the scientific requirements for the follow-up of Gaia alerts, e.g. in the area of supernovae or cataclysmic variables * Discussion of technical issues related with alert dissemination and follow-up feedback ---- During the interactive workshop we plan to bring together: * Experts on the Gaia mission, including Gaia Science Alerts * People responsible for telescopes around the globe * Astronomers experienced with observations of transient phenomena * Scientists and experts active in studying transient phenomena * Scientists involved in the distribution of alerts, e.g. from skyalert.org * Individuals interested in the outreach possibilities of Gaia Science Alerts be5c2b84f025e15e9990aad909386deb1f105493 708 706 2011-02-21T10:12:26Z Lukasz 2 wikitext text/x-wiki The [[Workshop2010:main|first workshop on Gaia Science Alerts]], was held in June 2010 in Cambridge. We introduced the Science Alerts concept to a broad group of scientists from the international astronomical community. During the workshop key areas of interest were defined, and potential Gaia contributions to these fields were discussed in detail. '''All the talks and presentations are archived and available [[Workshop2010:agenda|here]].''' The Gaia Science Alerts stream will be the first Gaia data released to the community, so it is extremely important to produce reliable and robust alerts. To ensure that the released alerts are accurately classified, low in contaminants and contain interesting transient events, the complex data processing pipeline has to be thoroughly tested. The first alerts will need to be verified with an extensive programme of dedicated follow-up observations. These comprise: * imaging to confirm the presence and brightness of an alerting source, * continuous photometric monitoring to obtain a detailed light-curve to help fine-tune the classification * high/intermediate resolution spectroscopy to investigate the real nature of an event. ---- The verification programme is scheduled to take place in the first three months of operation of the Gaia Science Alert system. To classify as many alerts as possible requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close (mid-2013), we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. This meeting is the best way to achieve our primary goals: * Familiarisation of potential observers and research groups with Gaia and its alerting system, and the specific requirements of verification. * Prepare a plan of the detailed scope of the alerts verification phase, including how long it should last * Selection of likely telescopes and instruments * Identification of key people who will assist with verification * Confirmation of the scientific requirements for the follow-up of Gaia alerts, e.g. in the area of supernovae or cataclysmic variables * Discussion of technical issues related with alert dissemination and follow-up feedback ---- During the interactive workshop we plan to bring together: * Experts on the Gaia mission, including Gaia Science Alerts team * People responsible for telescopes around the globe * Astronomers experienced with observations of transient phenomena * Scientists and experts active in studying transient phenomena * Scientists involved in the distribution of alerts, e.g. from skyalert.org * Individuals interested in the outreach possibilities of Gaia Science Alerts 80902420267b51cf966f464a5fbfaca42681b7ea 713 708 2011-03-11T14:57:01Z Lukasz 2 wikitext text/x-wiki The [[Workshop2010:main|first workshop on Gaia Science Alerts]], was held in June 2010 in Cambridge. We introduced the concept of the Science Alerts to a broad group of scientists from the international astronomical community. During the workshop key areas of interest were defined, and potential Gaia contributions to these fields were discussed in detail. '''All the talks and presentations are archived and available [[Workshop2010:agenda|here]].''' The Gaia Science Alerts stream will be the first Gaia data released to the community, so it is extremely important to produce reliable and robust alerts. To ensure that the released alerts are accurately classified, low in contaminants and contain interesting transient events, the complex data processing pipeline has to be thoroughly tested. The first alerts will need to be verified with an extensive programme of dedicated follow-up observations. These comprise: * imaging to confirm the presence and brightness of an alerting source, * continuous photometric monitoring to obtain a detailed light-curve to help fine-tune the classification * high/intermediate resolution spectroscopy to investigate the real nature of an event. ---- The verification programme is scheduled to take place in the first three months of operation of the Gaia Science Alert system. To classify as many alerts as possible requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close (mid-2013), we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. This meeting is the best way to achieve our primary goals: * Familiarisation of potential observers and research groups with Gaia and its alerting system, and the specific requirements of verification. * Prepare a plan of the detailed scope of the alerts verification phase, including how long it should last * Selection of likely telescopes and instruments * Identification of key people who will assist with verification * Confirmation of the scientific requirements for the follow-up of Gaia alerts, e.g. in the area of supernovae or cataclysmic variables * Discussion of technical issues related with alert dissemination and follow-up feedback ---- During the interactive workshop we plan to bring together: * Experts on the Gaia mission, including Gaia Science Alerts team * People responsible for telescopes around the globe * Astronomers experienced with observations of transient phenomena * Scientists and experts active in studying transient phenomena * Scientists involved in the distribution of alerts, e.g. from skyalert.org * Individuals interested in the outreach possibilities of Gaia Science Alerts b7bfa21ab819272388449ddfdd54d9a262d89a15 0 106 707 654 2011-02-17T09:38:12Z Lukasz 2 wikitext text/x-wiki =Workshop's agenda= <center> <big>Post-workshop White Book is available [[Media:Postgsaw_wb.pdf|here]]</big></center> Abstract book can be downloaded [[Media:gsaw-abstract_book.pdf|here]]. The titles are linked to pdf versions of the talks. All presentations were also video recorded and are available in AVI format. {| style="border-color: #000; border-style: solid; border-width: 1px 1px 1px 1px; border-spacing: 0; border-collapse: collapse; margin: 0; padding: 4px;" |- |colspan="5"|<big>'''Wednesday 23 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee and registration </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Welcome address [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Kennicut-Welcome.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rob Kennicut |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/walton-great-wga5-jun10.pdf Welcome and update on GREAT] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Walton-IntroGREAT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nick Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia status | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Timo Prusti |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mignard_Science_Alerts_06_2010.pdf The Gaia mission: a primer] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mignard-MissionPrimer.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Francois Mignard |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/ScienceAlerts.pdf Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/LW-STH-ScienceAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | LW/STH |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Asteroid Alerts [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanga-Asteroids.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paolo Tanga |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Smartt-GAIA-Alerts.pdf Transient and Supernovae searches with PS1] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Smartt-Panstarrs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Stephen Smartt |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:25 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/obrien-gaia-june2010.pdf High energy transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/OBrien-HighEnergyTransients.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Paul O&#39;Brien |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wozniak-gsaw_2010.pdf Explosive Transient Detection in the Era of Synoptic Sky Surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wozniak-Raptor.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Przemek Wozniak |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Ofek-PTF_Results_GAIA_2010.pdf The Palomar Transient Factory] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ofek-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Eran Ofek |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/poznanski_gaia_talk.pdf PTF - The reduction, subtraction, detection, and classification pipelines + some results] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Poznanski-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Dovi Poznanski |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/wheatley.pdf Optical transients detected by the Wide Angle Search for Planets (WASP)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Wheatley-Wasp.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Peter Wheatley |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mahabal_Cambridge_GAIA_alertsp.pdf Real-time Transient classification, follow-up and the way forward] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mahabal-ReadTime.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ashish Mahabal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:05 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/QA-Surveys.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 1'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 19:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Reception and dinner in Churchill College </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Thursday 24 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Surveys | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/sullivan_gaiameeting_jun2010_web.pdf Gaia in the context of low-redshift transient surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Sullivan-GaiaInContext.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Mark Sullivan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/gal-yam-gaia-UK-2010.pdf The PTF core-collapse supernova key project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/GalYam-PTF.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Avishay Gal-Yam |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Turrato_GaiaAlert_Cambr2010.pdf Supernova monitor programs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Turatto-Supernovae.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Massimo Turatto |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Variability, outbursts and mass loss amongst massive evolved stars [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Clark-MassiveStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Simon Clark |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tanvir-Gaia-GRBs.pdf GRB science with GAIA] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tanvir-GRBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Nial Tanvir |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Orphan GRB afterglows with GAIA [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Levan-GRBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Levan |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gould-microlensing_alerts.pdf Gaia Microlensing Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Gould-Microlensing.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Andrew Gould |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Dominik-Microlensing-LiveColour_slides.pdf Microlensing live and in colour] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Dominik-Microlensing.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Dominik |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [[Media:GaiaScienceAlertsWorkshop2010photo.jpg|Workshop photo]] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steeghs_Cambridge_GAIA_Jun10.pdf Accretion-driven transients in the Galaxy] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Steeghs-Acretion.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Danny Steeghs |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Gaensicke-CVs.pdf The galactic population of cataclysmic variables] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Gaensicke-CVs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Boris Gaensicke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/kospal_gaia.pdf Irregular variability during early stellar evolution: what can we learn about the circumstellar material?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Kospal-Irregular.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Agnes Kospal |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Tisserand_RCB_AlertGAIA2010 R Coronae Borealis variability and Galactic distribution (and SkyMapper)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Tisserand-RCBs.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Patrick Tisserand |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Tea </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Science | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion/Summary''' [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/QA-Science.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Outreach possibilties with Gaia and Hands-On-Universe [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Ferlet-HandsOnUniverse.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Roger Ferlet |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 16:55 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Mankiewicz-Gaia_2010.pdf Outreach/Citizen's Science potential of GAIA Science Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Mankiewicz-Outreach.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Lech Mankiewicz |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:20 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | '''Q+A/Discussion''' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 17:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 2'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- |- |colspan="5"|<big>'''Friday 25 June 2010'''</big> |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''time'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''session'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''title'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''speaker'' |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Gaia | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altmann-gsa_cambridge10.pdf Ground Based Optical Tracking of Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Altmann-GBOT.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Martin Altmann |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 09:50 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Eyer-GSAW.pdf Gaia and variable stars ; Ground based follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Eyer-VariableStars.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Laurent Eyer |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:15 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Hudec_Cambridge_10_ShortFinal3.pdf High-Energy Sources and Cataclysmic Variables as Alert Targets for Gaia. Major spectral changes from BP/RP] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Hudec-CVsSpectra.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Rene Hudec |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 10:40 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Seabroke_gaia_alerts_cambridge.pdf How Gaia's Radial Velocity Spectrometer (RVS) can contribute to Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Seabroke-RVSAlerts.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | George Seabroke |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA500"> Coffee </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:30 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Alert distribution possibilities | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Ross Burgon |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 11:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Follow-up | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Lewis-followup.pdf Follow-up opportunities with robotic telescopes] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Lewis-Followup.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Fraser Lewis |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:10 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/steele-lt-gaia-transient.pdf Transient Astronomy with the Liverpool Telescope: Software, Systems and Science] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Steele-Liverpool.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Iain Steele |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 12:35 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/naylor-estar.pdf The eSTAR Project] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/Naylor-eStar.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Tim Naylor |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 13:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | <span style="color:#FFA07A"> Lunch </span> | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | Discussion | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/great-wga5-jun10-walton-close.pdf '''Discussion - towards the Road Map'''] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Movies/ClosingDiscussion-Summary.avi recording] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | led by N.Walton |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 14:45 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/GSAW2010-summary.pdf '''Concluding summary'''] | style="border-width: 0px 1px 1px 0px; border-style: solid;" | All |- | style="border-width: 0px 1px 1px 0px; border-style: solid;" | 15:00 | style="border-width: 0px 1px 1px 0px; border-style: solid;" | | style="border-width: 0px 1px 1px 0px; border-style: solid;" | ''end of day 3'' | style="border-width: 0px 1px 1px 0px; border-style: solid;" | |} Posters: Giuseppe Altavilla, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2010/Talks/Altavilla-GaiaAlerts-poster.pdf Gaia and discovery of Supernovae] 9c5b368a5129b5434ecafb731bc17b6eee347667 0 138 709 2011-02-21T10:20:14Z Lukasz 2 Created page with 'The workshop stars in late morning on Wednesday 29th of June and will conclude after lunch on Friday, 1st July. The agenda will comprise on presentation of Gaia and Gaia alerts ...' wikitext text/x-wiki The workshop stars in late morning on Wednesday 29th of June and will conclude after lunch on Friday, 1st July. The agenda will comprise on presentation of Gaia and Gaia alerts stream, brief outline of scientific topics to which Gaia alerts can contribute, presentations of existing and future transient surveys and follow-up teams and telescopes. The final scope of the agenda, however, will be decided based on the suggested contributions from the participants. The workshop's dinner will probably take place in St.John's Chop House on Thursday evening. e13f410e6d4e782331dc42c4974a6abc5e6a4f67 0 11 710 675 2011-03-01T14:30:25Z Lukasz 2 /* Preliminary list of telescopes and people involved */ wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] f6371d24e11ec7c7f6f828a1660dc344d60ac022 0 131 714 699 2011-03-23T16:36:21Z Lukasz 2 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. [[File:Poster.jpn]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss d61061d8eb7434f9995bd1facb624bf310d566c6 715 714 2011-03-23T16:36:36Z Lukasz 2 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. [[File:Poster.jpg|right]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss f6afa9b1ebddcc48fd415fec8fad2f37dffa95c8 716 715 2011-03-25T09:21:37Z Lukasz 2 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. This time we will concentrate on the crucial issues the verification and follow-up of the Gaia alerts. We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster.jpg|right]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss b3f11a012871d599a7a294b8ebe69f3dd64bce4f 717 716 2011-03-25T09:21:49Z Lukasz 2 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. This time we will concentrate on the crucial issues the verification and follow-up of the Gaia alerts. We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster.jpg|right]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss 97ddb1939b7772b0e3ebcf38bfbda7d9604e566e 718 717 2011-03-25T11:20:07Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. This time we will concentrate on the crucial issues the verification and follow-up of the Gaia alerts. We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster.jpg|right]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] * [[workshop2011:poster]|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss 7814ed2928633f62f9df8d47db34a58576dab8bc 719 718 2011-03-25T11:20:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. This time we will concentrate on the crucial issues the verification and follow-up of the Gaia alerts. We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster.jpg|right]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] * [[workshop2011:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss 754bd5bd9712e2cd9a5759387376eae00d5e2da2 730 719 2011-03-28T15:53:51Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == The second Gaia Science Alerts workshop will be held in Cambridge between June 29th and 1st July 2011. This time we will concentrate on the crucial issues the verification and follow-up of the Gaia alerts. We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster.jpg|right|300px]] ---- * [[workshop2011:rationale|Rationale]] * [[workshop2011:agenda|Agenda]] * [[workshop2011:registration|Registration]] * [[workshop2011:logistics|Logistic information]] * [[workshop2011:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Floor van Leeuven * Judith Moss d753f8e360905d94e339749d1cdc5ee25dd35e5f 0 139 720 2011-03-25T11:20:53Z Gsawgwikiadmin 1 Created page with 'Poster in the [File:GaiaWorkshop2011poster.pdf|PDF]' wikitext text/x-wiki Poster in the [File:GaiaWorkshop2011poster.pdf|PDF] a33c43acd2a7fc45c2441a31925fb9d020817a33 721 720 2011-03-25T11:21:00Z Gsawgwikiadmin 1 wikitext text/x-wiki Poster in the [[File:GaiaWorkshop2011poster.pdf|PDF]] 05a2d5630bab0a5bbe3e3967b45302cf9e4b7ac6 722 721 2011-03-25T11:33:28Z Gsawgwikiadmin 1 wikitext text/x-wiki Poster in the [[File:GaiaWorkshop2011poster.pdf PDF]] d687fbd7347f3594d1a492568772a2d708adfa3a 723 722 2011-03-25T11:33:35Z Gsawgwikiadmin 1 wikitext text/x-wiki Poster in the [File:GaiaWorkshop2011poster.pdf PDF] 1585836a21d279fb1a236860ac4cdc7fc6e1da9c 724 723 2011-03-25T11:33:52Z Gsawgwikiadmin 1 wikitext text/x-wiki Poster in the [[Media:GaiaWorkshop2011poster.pdf PDF]] 9768bf0f014a7563a35ba8fe8204d12e196eb188 725 724 2011-03-25T11:33:58Z Gsawgwikiadmin 1 wikitext text/x-wiki Poster in the [[Media:GaiaWorkshop2011poster.pdf|PDF]] 3a867284a7e9c47c9252462e70996ecef0c07beb 733 725 2011-03-28T16:01:45Z Gsawgwikiadmin 1 wikitext text/x-wiki Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf| PDF]. Smaller version in [[Media:GaiaAlerts2011-poster.jpg| JPG]]. [[File:Poster.jpg|right|400px]] 91fa350520f61245013d3bd81763e45c433528df 734 733 2011-03-28T16:02:29Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster.jpg|right|400px]] <big>'''We would appreciate if you could print the poster and display it in your institute.'''</big> Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf| PDF]. Smaller version in [[Media:GaiaAlerts2011-poster.jpg| JPG]]. 4084a462a2cc9b81dc63e186892de284f0dd9093 735 734 2011-03-28T16:02:40Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster.jpg|right|400px]] <big>'''We would appreciate if you could print the poster and display it in your institute.'''</big> * Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf| PDF]. * Smaller version in [[Media:GaiaAlerts2011-poster.jpg| JPG]]. e98ed56dd827dfd68c0cbe916599c6a37ad2dc47 736 735 2011-03-28T16:03:10Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster.jpg|right|400px]] <big>'''We would appreciate if you could print the poster and display it in your institute.'''</big> * Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf| PDF]. * Smaller version in [[Media:Poster.jpg| JPG]]. efafae6be76a1e533f4452873a3d95a89014ecaa 737 736 2011-03-28T16:03:31Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster.jpg|right|400px]] <big>'''We would appreciate if you could print the poster and display it in your institute.'''</big> * Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf PDF]. * Smaller version in [[Media:Poster.jpg| JPG]]. da0db3b68089e77a41b2200f4a33096d8326a699 738 737 2011-03-28T16:04:04Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster.jpg|right|400px]] <big>'''We would appreciate if you could print the poster and display it in your institute.'''</big> * Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf PDF] (1.7MB) * Smaller version in [[Media:Poster.jpg| JPG]] (650kB) c4e35fedc290f8d93b7a8c0e1bf03f8015a63bdb 739 738 2011-03-28T16:04:43Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster.jpg|right|400px]] <big>'''Please print the poster and display it in your institute.'''</big> * Poster in the [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/GaiaAlerts2011-poster.pdf PDF] (1.7MB) * Smaller version in [[Media:Poster.jpg| JPG]] (650kB) 213fed26fa761da2b275a1bfc57ee4d0de8e993f 0 141 727 2011-03-28T15:28:08Z Gaia 3 Created page with 'Hello' wikitext text/x-wiki Hello f7ff9e8b7bb2e09b70935a5d785e0cc5d9d0abf0 6 142 728 2011-03-28T15:37:36Z Gaia 3 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 143 729 2011-03-28T15:53:07Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 144 731 2011-03-28T15:53:51Z Gaia 3 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 145 732 2011-03-28T15:54:13Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 146 740 2011-03-30T13:49:53Z Jure.Japelj 24 A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. wikitext text/x-wiki A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. d7f839e0b52b50c951ae0f5d378bba3600ecdc9f 741 740 2011-03-30T13:50:25Z Jure.Japelj 24 uploaded a new version of "[[File:Kann afterglow.pdf]]": A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. wikitext text/x-wiki A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. d7f839e0b52b50c951ae0f5d378bba3600ecdc9f 743 741 2011-03-30T17:50:06Z Jure.Japelj 24 uploaded a new version of "[[File:Kann afterglow.pdf]]": A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. wikitext text/x-wiki A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. d7f839e0b52b50c951ae0f5d378bba3600ecdc9f 6 147 742 2011-03-30T13:53:47Z Jure.Japelj 24 The average GRB on-axis afterglow detection rate in five years. wikitext text/x-wiki The average GRB on-axis afterglow detection rate in five years. fe5b0acd7640d486c0e3bcc49fa3139e983c4149 748 742 2011-03-31T09:20:51Z Jure.Japelj 24 uploaded a new version of "[[File:F1.pdf]]" wikitext text/x-wiki The average GRB on-axis afterglow detection rate in five years. fe5b0acd7640d486c0e3bcc49fa3139e983c4149 0 73 744 337 2011-03-30T17:51:05Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Short-lived optical transients associated with enormous gamma-ray outbursts GRBs. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * Time-scales of the gamma-ray emission range from a fraction of second to several minutes. This emission is often accompanied by the so-called optical afterglow which can last for several days. Optical afterglows can be therefore detected with Gaia even several days after the GRB trigger. * Optical afterglow can reach up to few mag in maximum, but the whole range of magnitudes observed at a given time elapsed from the GRB largely differs for the individual events (more than 3 mag). These optical afterglows often display specific color indices with negligible time evolution, which helps distinguish them from other kinds of transients by photometric observations using several color filters. * Host galaxy of GRB can be visible, but its apprent magnitude is usually fainter than the detection limit of Gaia (about 20 mag). Nevertheless, this host galaxy can often be detected by large ground-based telescopes at the position of the optical afterglow. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 0ae7beb2929b5afc8280817a3964f6a4e1ce646a 746 744 2011-03-30T17:53:33Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Short-lived optical transients associated with enormous gamma-ray outbursts GRBs. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * Time-scales of the gamma-ray emission range from a fraction of second to several minutes. This emission is often accompanied by the so-called optical afterglow which can last for several days. Optical afterglows can be therefore detected with Gaia even several days after the GRB trigger. * Optical afterglow can reach up to few mag in maximum, but the whole range of magnitudes observed at a given time elapsed from the GRB largely differs for the individual events (more than 3 mag). These optical afterglows often display specific color indices with negligible time evolution, which helps distinguish them from other kinds of transients by photometric observations using several color filters. * Host galaxy of GRB can be visible, but its apprent magnitude is usually fainter than the detection limit of Gaia (about 20 mag). Nevertheless, this host galaxy can often be detected by large ground-based telescopes at the position of the optical afterglow. [[File:kann_afterglow1.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. a98fa338082c5c4695908ff39d05849f57080486 747 746 2011-03-30T18:14:31Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Short-lived optical transients associated with enormous gamma-ray outbursts GRBs. A catalogue of GRBs is available [http://grad40.as.utexas.edu here]. Comprehensive recent review on GRBs and their physics can be found in [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] * Time-scales of the gamma-ray emission range from a fraction of second to several minutes. This emission is often accompanied by the so-called optical afterglow which can last for several days. Optical afterglows can be therefore detected with Gaia even several days after the GRB trigger. * Optical afterglow can reach up to few mag in maximum, but the whole range of magnitudes observed at a given time elapsed from the GRB largely differs for the individual events (more than 3 mag). These optical afterglows often display specific color indices with negligible time evolution, which helps distinguish them from other kinds of transients by photometric observations using several color filters. * Host galaxy of GRB can be visible, but its apprent magnitude is usually fainter than the detection limit of Gaia (about 20 mag). Nevertheless, this host galaxy can often be detected by large ground-based telescopes at the position of the optical afterglow. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 0ae7beb2929b5afc8280817a3964f6a4e1ce646a 6 148 745 2011-03-30T17:52:56Z Jure.Japelj 24 A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. wikitext text/x-wiki A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. d7f839e0b52b50c951ae0f5d378bba3600ecdc9f 6 149 749 2011-03-31T13:45:46Z Jure.Japelj 24 A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. wikitext text/x-wiki A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction. d7f839e0b52b50c951ae0f5d378bba3600ecdc9f 6 150 750 2011-03-31T13:46:33Z Jure.Japelj 24 The average GRB on-axis afterglow detection rate in five years. wikitext text/x-wiki The average GRB on-axis afterglow detection rate in five years. fe5b0acd7640d486c0e3bcc49fa3139e983c4149 6 151 751 2011-03-31T13:47:20Z Jure.Japelj 24 The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments. wikitext text/x-wiki The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments. a82d79f0b5d5dfc33e2608dd703cd5d3000cab4f 6 152 752 2011-03-31T13:48:47Z Jure.Japelj 24 Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red). wikitext text/x-wiki Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red). 9b05fd34318f908c4f074e3f214aa07997735ad5 6 153 753 2011-03-31T13:49:24Z Jure.Japelj 24 Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray). wikitext text/x-wiki Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray). 9157a4684a64f6e8d7f24fcbaa5a54cc234397cd 0 73 754 747 2011-03-31T13:56:16Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle $\theta_{j}$. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. f1cc7c9b4fd80081107b8401ae352c978aa0112c 755 754 2011-03-31T13:56:54Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 8569546b640a6f36950a547b6547f42a0c450ea1 756 755 2011-03-31T13:58:07Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>\theta_{j}</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 6e48e8ba7ea10e5c5ed7e4eddea1bca348d17796 757 756 2011-03-31T13:59:43Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>\theta_j</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 88267f0a053e96f40f28beb4364dd6c5e38122ac 758 757 2011-03-31T14:02:22Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>\theta\,\!_j</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 78762fcb93918e7d4f58678883ae99d6ccd21f11 759 758 2011-03-31T14:02:34Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>t_j</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 2225ec5f841bedaf887ce0bfe05284745e2f9448 760 759 2011-03-31T14:03:00Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math> t_{j} </math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 368a5a118d927b2cfe1f027c3515c2c965014211 761 760 2011-03-31T14:03:36Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle &theta. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 8835aaf236fe31c428780dd8b6bca38975db4d6c 762 761 2011-03-31T14:04:53Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>T \propto R^{-3/4}</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. d973addd96ce88231cf87d21fbce84ed85d75e3f 763 762 2011-03-31T14:05:21Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>\theta</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 72d15a489d16fa7f5181e81299f3f35cd19b42f7 764 763 2011-03-31T14:05:59Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>\theta\,\!</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. bd9a477aef304f7812fb0046c6f69944ccfc73a3 765 764 2011-03-31T14:09:13Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>t_{j}</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 2763c51666daf8bc0870bf78bac43f0baef633f0 766 765 2011-03-31T14:10:17Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle {{math|<VAR>&alpha;</VAR>}}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 8e6cd45c9621f819cee4b981c4836f1ea0de54ae 767 766 2011-03-31T14:11:17Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>t_j</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 2225ec5f841bedaf887ce0bfe05284745e2f9448 768 767 2011-03-31T14:12:55Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>t _ j</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. db52374446f375190ef33db48959dfa53ee1e56c 769 768 2011-03-31T14:13:12Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>t^j</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 0acf2fb296212844c821d15974b1ebc70b946a18 770 769 2011-03-31T14:15:08Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle <math>a</math>. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. A large sample of observed optical lightcurves is shown in Figure 2. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. ccdcafd008a9a84ca10bb98d8d734afe1bb85acc 771 770 2011-03-31T14:25:24Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. [[File:kann.png|300px|right]] A large sample of observed optical lightcurves is shown in Figure on right [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 4b6acaaa5af53f2cc139b97bce6b6a17407ea607 772 771 2011-03-31T14:26:14Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. [[File:kann.png|300px|left]] A large sample of observed optical lightcurves is shown in Figure on right [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]. Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. ee4a4e5a1eec0521dca3b8d2cc735b0146f5a21c 773 772 2011-03-31T14:26:51Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves is shown in Figure on left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 31e47b0111ac0c60d06f5826cd330b0485ee8ec9 774 773 2011-03-31T14:29:47Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in Figure on left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). [[File:Color-oa.png|400px|right]] It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. [[File:kann_afterglow.pdf|400px]] from [http://ukads.nottingham.ac.uk/abs/2006ApJ...642L..99W Wozniak et al. 2006] [[File:GRB08-PI.png|400px]] from [http://arxiv.org/abs/0903.2998 Sokolowski et al.2009] == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 800f7034a0c086536578fdcd5262ae086790c618 775 774 2011-03-31T14:30:26Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in Figure on left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). [[File:Color-oa.png|300px|right]] It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. b58b87e90f7e9385babd33445a5b616b69a49521 776 775 2011-03-31T14:31:17Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in Figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in Figure on left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|300px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognise an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 0014f011bb039f0b4687348bd0e842f8da74040a 777 776 2011-03-31T14:33:04Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|300px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|300px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. eeb299f64f711f122fb8a9684da30b06017bc373 778 777 2011-03-31T14:33:50Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. e8bf7e9b390e25f7080299acd9f70020f9231219 779 778 2011-03-31T14:38:43Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. \vspace == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 6292c98d6fafd4c57d334c4a0c0d419c5623f33e 780 779 2011-03-31T14:39:16Z Jure.Japelj 24 wikitext text/x-wiki [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. <math>\vspace{2cm}</math> == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 161d05d22278146e8834e68ce0d2211c736926ff 781 780 2011-03-31T14:40:31Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A$\%$26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. 57ca2a1b2da615cfc8a4a1561b36ce7ca4feb3bd 782 781 2011-03-31T14:41:29Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. == Detecting GRBs with Gaia == [[File:plot_grb_eff.png|400px|Thumb|right|Gaia detection efficiency for GRBs in per cents.]] About 5% of GRBs is detectable by Gaia, with the highest efficiency close to the nodes. The main feature visible in the data is steady and rapid decline over AF CCDs. Time sampling at AF CCDs level is 4.4s per CCD. We also demand the transient to be visible in the second FOV (after 105 min). [[File:plot_grb_mag_15.png|400px|left]] [[File:plot_grb_mag.png|400px|right]] [[File:GRB-fraction.png|300px]] from [http://prola.aps.org/abstract/RMP/v76/i4/p1143_1 Piran,2005] [[File:Color-oa.png|400px|left]] Color-color (''B-V'' vs. ''V-R'') diagram of optical afterglows of long GRBs. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble ([http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004]) are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for ''E(B-V)'' = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Simon et al., 2001], [http://adsabs.harvard.edu/abs/2004AIPC..727..487S 2004], where a detailed information can be found. a3b2ebeaad0dfd069392a7d727fb6c8438e76f70 783 782 2011-03-31T14:45:25Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices $(R - I)$, $(V -R)$ and $(B - V)$ of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == 2d9a84af34ca5b6f7f641e0930f39fb849a6723d 784 783 2011-03-31T14:46:11Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == 022010e270ba125e23d714e340fa0b93dee0d3d2 785 784 2011-03-31T14:57:45Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|325px|right]] [[File:F2.jpg|325px|right]] Number of detections in respect to limiting magnitude are shown in Figure 4 and Figure 5. 420b2b20ca624d09825e65eb37a53d1e4c3e07ee 786 785 2011-03-31T14:58:39Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|500px|right]] [[File:F2.jpg|500px|right]] Number of detections in respect to limiting magnitude are shown in Figure 4 and Figure 5. ae6bf65bbcf8f13ca6f2b7195835e740a23e9de4 787 786 2011-03-31T14:59:06Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|450px|right]] [[File:F2.jpg|450px|right]] Number of detections in respect to limiting magnitude are shown in Figure 4 and Figure 5. d6f4bc9d26fe51c9deced353ecea0cfb368063ca 788 787 2011-03-31T15:00:54Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|450px|right]] [[File:F2.jpg|450px|right]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. d8ee80b1ef7f1bf4c322d91445ef501f22fd657a 789 788 2011-03-31T15:02:28Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|450px|right]] [[File:F2.jpg|450px|right]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. [[File:F3.jpg|450px|left]] Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. 55ac05667bc01c03f34bedad9167cc66c1b11b3a 790 789 2011-03-31T15:03:13Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. [[File:F3.jpg|400px|left]] Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. 077ef63c1205fdfefaaa50d5083de59cb4aea00a 791 790 2011-03-31T15:03:56Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. 10f543ef025cf19d9d278b2fa17898c0f0834204 792 791 2011-03-31T15:04:53Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. [[File:F2.jpg|400px|right]] [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|left]] 56d61424d52be02a137f09daf7f20fa825257123 793 792 2011-03-31T15:05:28Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|left]] f88e65b9cf214774360f9a4b19ec560ba6cdba09 794 793 2011-03-31T15:07:14Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. [[File:F3.jpg|400px|left]] Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. [[File:F4.jpg|400px|left]] 4533720d60226541c9f504fdf0c254324ab1ea3a 795 794 2011-03-31T15:07:54Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|right]] 05c2bdb540d9e1389742199521495cd466965858 796 795 2011-03-31T15:09:48Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|right]] 5111689184046dd814575d8ff3051a0cf5671e4b 797 796 2011-03-31T15:11:34Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|left]] Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. ba835637f234554b8bccea9c03426610119ca63d 798 797 2011-03-31T15:12:11Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. [[File:F3.jpg|400px|left]] [[File:F4.jpg|400px|left]] Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. 5f27c734f37ccba8924a28daf50d9fe6791e96ed 799 798 2011-03-31T15:15:21Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right]] [[File:F2.jpg|400px|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. [[File:F3.jpg|400px|border|left]] [[File:F4.jpg|400px|left]] Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. c1a49083fc50bac52775a84d6927389dcb6b34d6 800 799 2011-03-31T15:16:38Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|border|right]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. [[File:F3.jpg|400px|border|left]] [[File:F4.jpg|400px|border|left]] Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. 732d12ac34d51a01fbc184c605ce77def595d323 801 800 2011-03-31T15:17:32Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|border|right]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] [[File:F4.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. babf44d2d03fb311d78beca60a39d4b989901713 0 73 802 801 2011-03-31T15:19:16Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] [[File:F4.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. 938df65e14a3811a8fa456f1fe0888e7fb5700b9 803 802 2011-03-31T15:19:39Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|border|right|{The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.}]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] [[File:F4.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. 13a37302a107d513060745cfe428508e76397351 804 803 2011-03-31T15:22:16Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] [[File:F4.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. 36ba6b8f11c926a8d0aaf65a21122cd217005a13 805 804 2011-03-31T15:29:07Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. [[File:F4.jpg|400px|border|left]] To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. 4037ff4182739ec0347638a234071f3dd5fabed3 806 805 2011-03-31T15:29:30Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F4.jpg|400px|border|left]] c7ff57a691bc2d1b6899954aca917c05f8095774 807 806 2011-03-31T15:30:12Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and bottom figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Figure 6 shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in Figure 7. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. b1ba304a3cc0c0734158cd5a37cc6e37a1783354 808 807 2011-03-31T15:32:22Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. a3b852b0974668b73269a37e5e5e78aaaf3ea6b7 810 808 2011-03-31T18:07:01Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[User:Jure.Japelj|Jure.Japelj]] 18:07, 31 March 2011 (UTC) af4840ea5b68e339141c4d5abd34a68321c97b1a 811 810 2011-03-31T18:08:46Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[User:Username|Jure Japelj]] 4d9645d0aad8cf377c3c1e7a05cedd951d3b820f 812 811 2011-03-31T18:09:43Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[User:Jure.Japelj|Jure.Japelj]] 18:09, 31 March 2011 (UTC) d02e9148e171d41771904faa87b748cc2fa30baf 813 812 2011-03-31T18:09:59Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 6a10a6b1064814ee955cfabeac6d76c889795e95 814 813 2011-03-31T18:13:14Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarise: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation details == [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) d6e2591679802a76964c2736724d94d532c81670 815 814 2011-03-31T18:17:40Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 2a50765a08bd97d133f3336acfc7aa8632598217 816 815 2011-03-31T18:20:43Z Jure.Japelj 24 /* Simulation references */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 87d37d2f261e43d15bfc257d0d10e805bfb522d6 817 816 2011-03-31T18:23:09Z Jure.Japelj 24 /* Detecting GRBs with Gaia */ wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left|baseline]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) aeeb270e7edf41e161ef5d6ebdda8fb3460c6564 818 817 2011-03-31T18:23:48Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left|text-bottom]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 49181325732de6ff8352e4bd623b2ff0a4504f09 819 818 2011-03-31T18:24:32Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. [[File:F3.jpg|400px|border|left|top]] Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 498faa07a8b2a99c0ba352ac8277e6b6327d9863 820 819 2011-03-31T18:25:14Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] [[File:F3.jpg|400px|border|left]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 71861df1a7482ea9017df2c04d25dc6990da5e1a 821 820 2011-03-31T18:25:53Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] [[File:F3.jpg|400px|border|left|top]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) eb196c9bd03347c2d0c2a5f0f14f7a3048b7d619 822 821 2011-03-31T18:26:33Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|350px|border|left]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|325px|border|right]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|right|border|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|400px|border|right]] [[File:F4.jpg|400px|border|right]] [[File:F3.jpg|400px|border|left|top]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 2d1fc6fb13a6b15bec2533c737078feef3a4aa68 823 822 2011-03-31T18:32:06Z Jure.Japelj 24 wikitext text/x-wiki == Gamma-Ray Burst Optical Afterglows == [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] [[File:F3.jpg|thumb|400px|border|left|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) ca2350b2c08440cd1112261acb62f52433c458e8 824 823 2011-03-31T18:41:42Z Jure.Japelj 24 /* Gamma-Ray Burst Optical Afterglows */ wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] [[File:F3.jpg|thumb|400px|border|left|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 52eb90c5b1e8973907fee0c41e8dab59ee2e9675 825 824 2011-03-31T18:42:41Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] [[File:F3.jpg|thumb|400px|border|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 58f2a7738a00757a301cc7d8ef72a7c3f1483355 826 825 2011-03-31T18:43:51Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) e641ad401aeb7e3defab3a5f19858b9a3a30db4b 827 826 2011-03-31T18:44:28Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] [[File:F3.jpg|thumb|400px|border|center|bottom|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) ec24de9131487f4449ae491927ec27dc89333527 828 827 2011-03-31T18:45:13Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 2def0e961de1bf87110eb8d84babf1139456b7ec 829 828 2011-03-31T18:47:31Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == **J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia **J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 83376a74172bed76b15f56575e223d440a67871d 830 829 2011-03-31T18:47:55Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in $\cite{japelj}$ and $\cite{japelj2}$, respectively. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 0cc1ecaa04812fcb32cc95e1323ca91a0ff83c7b 831 830 2011-03-31T18:50:21Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in $\cite{japelj2}$. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 16daffb5979567314ab80e30ec479131c4c7a2cb 832 831 2011-03-31T18:52:06Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 5209bba0aefbd0828bb93654edad7050635d395d 833 832 2011-03-31T18:52:45Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 84d07de3a36167d18a94c154be337bde593b4fbd 834 833 2011-03-31T18:58:31Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia <math>T \propto R^{-3/3}</math> [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 17971f1412cf7a408ad38ce002b7b4b6afada95d 835 834 2011-03-31T18:58:53Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia <math>T \propto R^{-3/4}</math> [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 5a562f51c5e48fd44e50a52ae4e8ab41b403f291 836 835 2011-03-31T19:01:32Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle \theta_{j}. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 6ab89c6768762a0e93deaac6eb347bd9cb8111f5 838 836 2011-03-31T19:02:59Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle $\theta_{\rm obs}$ between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when $\theta_{\rm obs} < \theta_{\rm j}$. In the case of $\theta_{\rm obs} > \theta_{\rm j}$, we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 010587b6cc59d880c99bbead9a138271e580ac59 842 838 2011-03-31T19:07:35Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 2f409b1862a2073515043ef756ba697bbb5b6a9c 843 842 2011-03-31T19:08:37Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 5c7ba627491702b2970a000428b4ff153ff4f7c1 844 843 2011-04-05T12:04:55Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia [http://www.fmf.uni-lj.si/~gomboc/report.pdf (download)] *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [http://www.fmf.uni-lj.si/~gomboc/reportOA.pdf (download)] [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) b96c194ce9b15f0ba0abdebc30d48e2c808f1cd5 845 844 2011-04-05T12:05:57Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia [http://www.fmf.uni-lj.si/~gomboc/report.pdf download] *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [http://www.fmf.uni-lj.si/~gomboc/reportOA.pdf download] [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 7ef3c92f1ad0334cc961334767bdbc2811b3ec7d 846 845 2011-04-05T12:06:59Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia [http://www.rssd.esa.int/index.php?project=GAIA&page=index download] *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [http://www.fmf.uni-lj.si/~gomboc/reportOA.pdf download] [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 0d136a46a31324f74ae807e0e11378bc73523da0 847 846 2011-04-05T12:07:44Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) cc7275d75a09367d872d20fdfac83e1fb96e97a6 848 847 2011-04-05T13:10:30Z Jure.Japelj 24 /* Simulation references */ wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == [http://www.fmf.uni-lj.si/~gomboc/report.pdf download] *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) aa71cb8e1137f9c5c7b73d7c02ea62fd3398e2e9 849 848 2011-04-05T13:10:53Z Jure.Japelj 24 /* Simulation references */ wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, The estimation of detectability of on-axis GRB optical afterglows with Gaia [http://www.fmf.uni-lj.si/~gomboc/report.pdf download] *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 06f911f1966b8ae5771a6012e9058274d9d31130 850 849 2011-04-05T13:13:28Z Jure.Japelj 24 /* Simulation references */ wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, [http://www.fmf.uni-lj.si/~gomboc/report.pdf The estimation of detectability of on-axis GRB optical afterglows with Gaia] *J. Japelj, A. Gomboc, 2011, The estimation of detectability of GRB optical orphan afterglows with Gaia [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) b8d4e60945f50fc5281fc6157a7eae217e478c0d 851 850 2011-04-05T13:14:06Z Jure.Japelj 24 /* Simulation references */ wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F1.jpg|thumb|400px|border|right|The average GRB on-axis afterglow detection rate in respect to limiting magnitude in five years.]] [[File:F2.jpg|thumb|400px|border|right|The average GRB orphan-afterglow detection rate in five years in the case of two different circumburst environments.]] [[File:F4.jpg|thumb|400px|border|right|Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change during the afterglow presence in the field of view (gray).]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details of on-axis and orphan afterglow simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top and the middle figure for the case of on-axis and orphan afterglows, respectively. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (but probably bigger [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected orphan afterglow detections with the Gaia satellite during it's five years of expected operation is of the order of 10. Adding the results of the on-axis afterglows simulation, the number of expected optical afterglow detections in five years is slightly increased. The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F3.jpg|thumb|400px|border|center|Distribution of initial magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (gray) and magnitudes of afterglows detected also by the second telescope (red).]] == Simulation references == *J. Japelj, A. Gomboc, 2011, [http://www.fmf.uni-lj.si/~gomboc/report.pdf The estimation of detectability of on-axis GRB optical afterglows with Gaia] *J. Japelj, A. Gomboc, 2011, [http://www.fmf.uni-lj.si/~gomboc/reportOA.pdf The estimation of detectability of GRB optical orphan afterglows with Gaia] [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 8b910f2ba41a9a7d9a7aeb4d7596d31d5e810afd 6 154 809 2011-03-31T15:38:36Z Jure.Japelj 24 Report on the simulation of the detectability of regular 'on-axis' GRB optical afterglows with the Gaia satellite. wikitext text/x-wiki Report on the simulation of the detectability of regular 'on-axis' GRB optical afterglows with the Gaia satellite. a3645ced5a952a8fa1e61ab41e7ab49e2508309e 6 155 837 2011-03-31T19:02:15Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 156 839 2011-03-31T19:05:56Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 157 840 2011-03-31T19:06:10Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 158 841 2011-03-31T19:06:23Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 135 852 712 2011-04-14T15:12:51Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. 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'''If you would like to attend the workshop please fill the form [[Workshop2011:registrationform | here]].''' </big> ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Kailash Sahu, STSI, USA # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK ea89d38ade7f406d0ffc99f0c3665a46f4a705fa 866 865 2011-06-02T09:05:22Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''The registration is now closed. The list of accepted participants is available below.''' ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Kailash Sahu, STSI, USA # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK e553d9958578b6a7704689afef94d487b12ed9c3 867 866 2011-06-03T11:41:49Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''The registration is now closed. The list of accepted participants is available below.''' ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Kailash Sahu, STSI, USA # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK # Martin Bell, Southampton, UK 88fa9d8b1237475216267c95061d01337edf1d33 868 867 2011-06-03T13:05:34Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''The registration is now closed. The list of accepted participants is available below.''' ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK # Martin Bell, Southampton, UK f171e6b6bdb2304ef62ca52fd84367d8e9ec07bf 869 868 2011-06-07T15:15:45Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''The registration is now closed. The list of accepted participants is available below.''' ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK # Martin Bell, Southampton, UK # Marcin Sokolowski, Warsaw, Poland 18f4cdbfec6e962989dda46f6b753f985104b7c3 888 869 2011-06-20T08:23:54Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''The registration is now closed. The list of accepted participants is available below.''' ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK # Martin Bell, Southampton, UK # Marcin Sokolowski, Warsaw, Poland # Lukasz Wyrzykowski, IoA, Cambridge, UK # Simon Hodgkin, IoA, Cambridge, UK # Floor van Leeuven, IoA, Cambridge, UK # Gerry Gilmore, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Vasily Belokurov, IoA, Cambridge, UK # Craig Mackay, IoA, Cambridge, UK 3f03d042bb42192aca8a1be9087a7f614f95e9f0 889 888 2011-06-20T08:24:17Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 30-35 attendees. The allocation of the places will be subject to registration application. '''The registration is now closed. The list of accepted participants is available below.''' ---- ==== List of Registered Participants ==== # Iain Steele, Liverpool, UK # Roy Williams, Caltech, USA # Yiannis Tsapras, LCOGT London, UK # Elsa Recillas, INAOE, Mexico # Massimo Turatto, Trieste, Italy # Neil Mawson, Liverpool, UK # Danny Steeghs, Warwick, UK # Gisella Clementini, Bologna, Italy # Paolo Tanga, Nice, France # Jan Soldan, Ondrejov, Czech Republic # Michel Dennefeld, IAP, France # William Thuillot, Paris Observatory, France # Jure Japelj, Univ. of Lubljana, Slovenia # Andreja Gomboc, Univ. of Lubljana, Slovenia # Peter Wheatley, Univ. of Warwick, UK # Svea Proft, Heidelberg, Germany # Martin Dominik, St. Andrews, UK # Utsav Kandel, Nepal # Ross Burgon, OU, UK # Giuseppe Altavilla, Bologna, Italy # Patricia Whitelock, SAAO, South Africa # Ashish Mahabal, Caltech, USA # Uffe Graae Jorgensen, Copenhagen, Denmark # Habib Khosroshahi, Tehran, Iran # Lech Mankiewicz, Warsaw, Poland # Laurent Eyer, Geneva, Switzerland # Stuart Littlefair, Sheffield, UK # Paola Di Matteo, Paris, France # Rene Hudec, Ondrejov, Czech Republic # George Seabroke, MSSL, UK # Martin Bell, Southampton, UK # Marcin Sokolowski, Warsaw, Poland # Lukasz Wyrzykowski, IoA, Cambridge, UK # Simon Hodgkin, IoA, Cambridge, UK # Floor van Leeuven, IoA, Cambridge, UK # Gerry Gilmore, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Vasily Belokurov, IoA, Cambridge, UK # Wyn Evans, IoA, Cambridge, UK # Craig Mackay, IoA, Cambridge, UK 3c8c7ee1b4d4ec692a332f441b3a5df589bd564f 0 1 854 690 2011-05-09T13:45:09Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>[[Workshop2011:main|Workshop 2011 - Gaia alerts verification and follow-up]]</Big> 29th June - 1st July 2011, Cambridge </center> ---- <center> [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010- archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 5d2ccc3094db16f1c33c401ab274ba6515431d96 0 159 870 2011-06-13T12:24:53Z Lukasz 2 Created page with "{| class="wikitable" | | |session |title |name |time (with discussion) |---- | |Wednesday | | | | |---- | |10:00 | |Welcome and technical |STH/LW |15m |---- | |10:15 |Gaia |Gaia ..." wikitext text/x-wiki {| class="wikitable" | | |session |title |name |time (with discussion) |---- | |Wednesday | | | | |---- | |10:00 | |Welcome and technical |STH/LW |15m |---- | |10:15 |Gaia |Gaia overview, include GBOT |FvL? |30m |---- | |10:45 | |Gaia Alerts overview |LW |30m |---- | |11:15 |coffee | | |30m |---- | |11:45 |Gaia |Asteroids |Paolo Tanga |30m |---- | |12:15 |Gaia |RVS alerts |Paola di Mateo |30m |---- | |12:45 |lunch | | |90m |---- | |14:15 |Science |Variable stars?? |Laurent Eyer |25m |---- | |14:40 | |SNe, overview and follow-up |Massimo Turrato? |25m |---- | |15:05 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |20m |---- | |15:25 | |tea | |35m |---- | |16:00 | |Microlensing |Dominik/Belokurov? |20m |---- | |16:20 | |GRBs |Jure Japelj |20m |---- | |16:40 | |CVs |Danny Steeghs |20m |---- | |17:00 | |High energy? |Rene Hudec? |20m |---- | |17:20 | |Exotics |Simon Hodgkin?? |20m |---- | |17:40 | | | | |---- | |Thursday | | | | |---- | |09:30 |Facilities |SONG |Uffe Jorgensen |20m |---- | |09:50 | |Java Robotic |Jan Soldan |20m |---- | |10:10 | |PI |Marcin Sokolowski |20m |---- | |10:30 | |Gloria |Lech Mankiewicz |20m |---- | |10:50 | |coffee | |40m |---- | |11:30 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- | |11:50 | |WASP |Peter Wheatley |20m |---- | |12:10 | |LCOGT |Yannis Tsapras |20m |---- | |12:30 | |lunch | |90m |---- | |14:00 | |STILT |Neil Mawson |20m |---- | |14:20 | |Liverpool |Iain Steele |20m |---- | |14:40 | |Iranian |Habib Khosroshahi |20m |---- | |15:00 | |PanStarrs & Spectroscopy |Stephen Smartt |30m |---- | |15:30 | |tea | |30m |---- | |16:00 | |Nepal |Utsav Kandel |20m |---- | |16:20 | |French facilities?? |Michel Dennefeld |20m |---- | |16:40 | |Italian facilities?? |Gisella Clementini |20m |---- | |17:00 | |other facilities?? |??? |20m |---- | |17:20 | |LOFAR |Martin Bell |30m |---- | |17:50 | | | | |---- | | | | | | |---- | | | | | | |---- | | | | | | |---- | |Friday | | | | |---- | |09:30 |Facilities |SAAO |Patricia Whitelock |30m |---- | |10:00 | |GBOG |George Seabroke |30m |---- | |10:30 | |Gaia-FUN |Whilliam Thuillot |30m |---- | |11:00 | |coffee | |30m |---- | |11:30 | |Catalina |Ashish Mahabal |30m |---- | |12:00 | |SkyAlert with demo |Roy Williams |30m |---- | |12:30 |Discussion |Getting organized |all |60m |---- | |13:30 | | | | |---- | |13:30 | | | | |---- |} c891ca4826bdaffafba575ce781b21388a788e94 871 870 2011-06-14T09:31:03Z Lukasz 2 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome and technical |STH/LW |15m |---- |10:15 |Gaia |Gaia overview |FvL? |30m |---- |10:45 | |Gaia Alerts overview |LW |30m |---- |11:15 |coffee | | |30m |---- |11:45 |Gaia |Asteroids |Paolo Tanga |30m |---- |12:15 |Gaia |RVS alerts |Paola di Mateo |30m |---- |12:45 |lunch | | |90m |---- |14:15 |Science |Variable stars?? |Laurent Eyer |20m |---- |14:35 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:05 | |Microlensing |Belokurov/Evans |20m |---- |15:25 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |35m |---- |16:00 | |tea | |20m |---- |16:20 | |GRBs |Jure Japelj |20m |---- |16:40 | | | |20m |---- |17:00 | |High energy? |Rene Hudec? |20m |---- |17:20 | |Exotics |Simon Hodgkin?? |20m |---- |17:40 | | | | |---- |Thursday | | | | |---- |09:30 | |Galactic transients and multi-wavelength synergies |Danny Steeghs |20m |---- |09:50 |Facilities |SONG |Uffe Jorgensen |20m |---- |10:10 | |Java Robotic |Jan Soldan |20m |---- |10:30 | |PI |Marcin Sokolowski |20m |---- |10:50 | |Gloria |Lech Mankiewicz |20m |---- |11:10 | |coffee | |40m |---- |11:50 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- |12:10 | |WASP |Peter Wheatley |20m |---- |12:30 | |LCOGT |Yannis Tsapras |20m |---- |12:50 | |lunch | |90m |---- |14:20 | |STILT |Neil Mawson |20m |---- |14:40 | |Liverpool |Iain Steele |20m |---- |15:00 | |Iranian |Habib Khosroshahi |20m |---- |15:20 | |tea | |40m |---- |16:00 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |16:30 | |Nepal facilities |Utsav Kandel |20m |---- |16:50 | |French facilities?? |Michel Dennefeld |20m |---- |17:10 | |Italian facilities?? |Gisella Clementini |20m |---- |17:30 | |other facilities?? |??? |20m |---- |17:50 | |LOFAR |Martin Bell |30m |---- |18:20 | | | | |---- | | | | | |---- |Friday | | | | |---- |09:30 |Facilities |SAAO |Patricia Whitelock |20m |---- |09:50 | |Opticon?? Outreach? |Gerry Gilmore |45m |---- |10:35 | |SkyAlert with demo |Roy Williams |20m |---- |10:55 | | | |30m |---- |11:25 | |GBOG |George Seabroke |30m |---- |11:55 | |Gaia-FUN |Whilliam Thuillot |30m |---- |12:25 | |coffee | |30m |---- |12:55 |Discussion |Catalina |Ashish Mahabal |60m |---- |13:55 | | | | |---- |13:55 | |Getting organized |all | |---- | | | | | |---- |} c6283e7dd298288bd7ad9766f5ce397ef1145ff5 872 871 2011-06-14T09:46:07Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome and technical |STH/LW |15m |---- |10:15 |Gaia |Gaia overview |FvL? |30m |---- |10:45 | |Gaia Alerts overview |LW |30m |---- |11:15 |coffee | | |30m |---- |11:45 |Gaia |Asteroids |Paolo Tanga |30m |---- |12:15 |Gaia |RVS alerts |Paola di Mateo |30m |---- |12:45 |lunch | | |90m |---- |14:15 |Science |Variable stars?? |Laurent Eyer |20m |---- |14:35 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:05 | |Microlensing |Belokurov/Evans |20m |---- |15:25 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |35m |---- |16:00 | |tea | |20m |---- |16:20 | |GRBs |Jure Japelj |20m |---- |16:40 | | | |20m |---- |17:00 | |High energy? |Rene Hudec? |20m |---- |17:20 | |Exotics |Simon Hodgkin?? |20m |---- |17:40 | | | | |---- |Thursday | | | | |---- |09:30 | |Galactic transients and multi-wavelength synergies |Danny Steeghs |20m |---- |09:50 |Facilities |SONG |Uffe Jorgensen |20m |---- |10:10 | |Java Robotic |Jan Soldan |20m |---- |10:30 | |PI |Marcin Sokolowski |20m |---- |10:50 | |Gloria |Lech Mankiewicz |20m |---- |11:10 | |coffee | |40m |---- |11:50 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- |12:10 | |WASP |Peter Wheatley |20m |---- |12:30 | |LCOGT |Yannis Tsapras |20m |---- |12:50 | |lunch | |90m |---- |14:20 | |STILT |Neil Mawson |20m |---- |14:40 | |Liverpool |Iain Steele |20m |---- |15:00 | |Iranian |Habib Khosroshahi |20m |---- |15:20 | |tea | |40m |---- |16:00 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |16:30 | |Nepal facilities |Utsav Kandel |20m |---- |16:50 | |French facilities?? |Michel Dennefeld |20m |---- |17:10 | |Italian facilities?? |Gisella Clementini |20m |---- |17:30 | |other facilities?? |??? |20m |---- |17:50 | |LOFAR |Martin Bell |30m |---- |18:20 | | | | |---- | | | | | |---- |Friday | | | | |---- |09:30 |Facilities |SAAO |Patricia Whitelock |20m |---- |09:50 | |Opticon?? Outreach? |Gerry Gilmore |20m |---- |10:10 | |SkyAlert with demo |Roy Williams |50m |---- |11:00 | |coffee | |30m |---- |11:30 | |GBOG |George Seabroke |20m |---- |11:50 | |Gaia-FUN |Whilliam Thuillot |25m |---- |12:15 | |Catalina |Ashish Mahabal |25m |---- |12:40 |Discussion |Getting organized |all |60m |---- |13:40 | | | | |---- |13:40 | | | | |---- | | | | | |---- |} 56178723df97d23ed689daa1efb641f91292b0a7 873 872 2011-06-14T11:00:23Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome and technical |STH/LW |15m |---- |10:15 |Gaia |Gaia overview |FvL? |30m |---- |10:45 | |Gaia Alerts overview |LW |30m |---- |11:15 |coffee | | |30m |---- |11:45 |Gaia |Asteroids |Paolo Tanga |30m |---- |12:15 |Gaia |RVS alerts |Paola di Mateo |30m |---- |12:45 |lunch | | |90m |---- |14:15 |Science |Variable stars?? |Laurent Eyer |20m |---- |14:35 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:05 | |Microlensing |Belokurov/Evans |20m |---- |15:25 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |35m |---- |16:00 | |tea | |20m |---- |16:20 | |GRBs |Jure Japelj |20m |---- |16:40 | | | |20m |---- |17:00 | |High energy? |Rene Hudec? |20m |---- |17:20 | |Exotics |Simon Hodgkin?? |20m |---- |17:40 | | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients and multi-wavelength synergies |Danny Steeghs |20m |---- |09:20 |Facilities |SONG |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic |Jan Soldan |20m |---- |10:00 | |PI |Marcin Sokolowski |20m |---- |10:20 | |Gloria |Lech Mankiewicz |20m |---- |10:40 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |WASP |Peter Wheatley |20m |---- |11:50 | |LCOGT |Yannis Tsapras |20m |---- |12:10 | |STILT |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |Liverpool |Iain Steele |20m |---- |14:20 | |Iranian |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Nepal facilities |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities?? |Gisella Clementini |20m |---- |16:50 | |LOFAR |Martin Bell |20m |---- |17:10 | |other facilities?? |??? |20m |---- |17:30 | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- |Friday | | | | |---- |09:30 |Facilities |SAAO |Patricia Whitelock |20m |---- |09:50 | |Opticon?? Outreach? |Gerry Gilmore |20m |---- |10:10 | |SkyAlert with demo |Roy Williams |50m |---- |11:00 | |coffee | |30m |---- |11:30 | |GBOG |George Seabroke |20m |---- |11:50 | |Gaia-FUN |Whilliam Thuillot |25m |---- |12:15 | |Catalina |Ashish Mahabal |25m |---- |12:40 |Discussion |Getting organized |all |60m |---- |13:40 | | | | |---- |} f700fdfe24d5bc2bc92355ecae21d9cbeedf613a 874 873 2011-06-14T11:20:23Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome and technical |STH/LW |15m |---- |10:15 |Gaia |Gaia overview |FvL? |30m |---- |10:45 | |Gaia Alerts overview |LW |30m |---- |11:15 |coffee | | |30m |---- |11:45 |Gaia |Asteroids |Paolo Tanga |30m |---- |12:15 |Gaia |RVS alerts |Paola di Mateo |30m |---- |12:45 |lunch | | |90m |---- |14:15 |Science |Variable stars?? |Laurent Eyer |20m |---- |14:35 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:05 | |Microlensing |Belokurov/Evans |20m |---- |15:25 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |35m |---- |16:00 | |tea | |20m |---- |16:20 | |GRBs |Jure Japelj |20m |---- |16:40 | | | |20m |---- |17:00 | |High energy? |Rene Hudec? |20m |---- |17:20 | |Exotics |Simon Hodgkin?? |20m |---- |17:40 | | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients and multi-wavelength synergies |Danny Steeghs |20m |---- |09:20 |Facilities |SONG |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic |Jan Soldan |20m |---- |10:00 | |PI |Marcin Sokolowski |20m |---- |10:20 | |Gloria |Lech Mankiewicz |20m |---- |10:40 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |WASP |Peter Wheatley |20m |---- |11:50 | |LCOGT |Yannis Tsapras |20m |---- |12:10 | |STILT |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |Liverpool |Iain Steele |20m |---- |14:20 | |Iranian |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Nepal facilities |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities?? |Gisella Clementini |20m |---- |16:50 | |LOFAR |Martin Bell |20m |---- |17:10 | |other facilities?? |??? |20m |---- |17:30 | | | | |---- |19:00 |DINNER at St.John’s Chop House | | | |---- | | | | | |---- |Friday | | | | |---- |09:30 |Facilities |SAAO |Patricia Whitelock |20m |---- |09:50 | |Engaging with the public |Gerry Gilmore |20m |---- |10:10 | |SkyAlert with demo |Roy Williams |50m |---- |11:00 | |coffee | |30m |---- |11:30 | |GBOG |George Seabroke |20m |---- |11:50 | |Gaia-FUN |Whilliam Thuillot |25m |---- |12:15 | |Catalina |Ashish Mahabal |25m |---- |12:40 |Discussion |Getting organized |all |60m |---- |13:40 | | | | |---- |13:40 | | | | |---- | | | | | |---- | | | | | |---- |} 94a77458378e38250826a03a72aa1bcd8b401508 877 874 2011-06-15T09:57:47Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome and technical |STH/LW |15m |---- |10:15 |Gaia |Gaia overview |FvL? |30m |---- |10:45 | |Gaia Alerts overview |LW |30m |---- |11:15 |coffee | | |30m |---- |11:45 |Gaia |Asteroids |Paolo Tanga |30m |---- |12:15 |Gaia |RVS alerts |Paola di Mateo |30m |---- |12:45 |lunch | | |90m |---- |14:15 |Science |Variable stars?? |Laurent Eyer |20m |---- |14:35 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:05 | |Microlensing |Belokurov/Evans |20m |---- |15:25 | |tea | |35m |---- |16:00 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |20m |---- |16:20 | |GRBs |Jure Japelj |20m |---- |16:40 | |High energy? |Rene Hudec? |20m |---- |17:00 | |Exotics |Simon Hodgkin?? |20m |---- |17:20 | | | |20m |---- |17:40 | | | | |---- | | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients and multi-wavelength synergies |Danny Steeghs |20m |---- |09:20 |Facilities |SONG |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic |Jan Soldan |20m |---- |10:00 | |PI |Marcin Sokolowski |20m |---- |10:20 | |Gloria |Lech Mankiewicz |20m |---- |10:40 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |WASP |Peter Wheatley |20m |---- |11:50 | |LCOGT |Yannis Tsapras |20m |---- |12:10 | |STILT |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |Liverpool |Iain Steele |20m |---- |14:20 | |Iranian |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Nepal facilities |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities?? |Gisella Clementini |20m |---- |16:50 | |LOFAR |Martin Bell |20m |---- |17:10 | |other facilities?? |??? |20m |---- |17:30 | |discussion? |all |30m |---- | | | | | |---- | | | | | |---- |Friday | | | | |---- |09:30 |Facilities |SAAO |Patricia Whitelock |20m |---- |09:50 | |Engaging with the public |Gerry Gilmore |20m |---- |10:10 | |SkyAlert with demo |Roy Williams |50m |---- |11:00 | |coffee | |30m |---- |11:30 | |GBOG |George Seabroke |20m |---- |11:50 | |Gaia-FUN |Whilliam Thuillot |25m |---- |12:15 | |Catalina |Ashish Mahabal |25m |---- |12:40 |Discussion |Getting organized |all |60m |---- |13:40 | | | | |---- |13:40 | | | | |---- | | | | | |---- | | | | | |---- |} d1647cff3f4ed6ecf746452ac03cdb2927e6fd8c 878 877 2011-06-15T17:03:02Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome and technical |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |FvL |25m |---- |10:35 | |Gaia Alerts overview |LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids |Paolo Tanga |25m |---- |12:00 |Gaia |RVS alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |GBOG |George Seabroke |20m |---- |14:15 | |Gaia-FUN |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Belokurov/Evans |20m |---- |16:20 | |Predicting Astrometric Microlensing for Gaia |Svea Proft |20m |---- |16:40 | |GRBs |Jure Japelj |20m |---- |17:00 | |High-z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotics? |Simon Hodgkin?? |20m |---- |17:40 |end of day 1 | | | |---- | | | | | |---- |19:00 |DINNER at St.John’s Chop House | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients and multi-wavelength synergies |Danny Steeghs |20m |---- |09:20 |Facilities |SONG |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic |Jan Soldan |20m |---- |10:00 | |PI |Marcin Sokolowski |20m |---- |10:20 | |Gloria |Lech Mankiewicz |20m |---- |10:40 | |Sheffield/Duram robotic 0.5m |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |WASP |Peter Wheatley |20m |---- |11:50 | |LCOGT |Yannis Tsapras |20m |---- |12:10 | |STILT |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |Liverpool |Iain Steele |20m |---- |14:20 | |Iranian |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Nepal facilities |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |LOFAR |Martin Bell |20m |---- |17:10 | |other facilities?? |??? |20m |---- |17:30 | |discussion? |all |30m |---- |18:00 |end of day 2 | | | |---- | | | | | |---- |Friday | | | | |---- |09:00 |Facilities |SAAO |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |Catalina |Ashish Mahabal |20m |---- |10:00 | |SkyAlert with demo |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 020ebac8c65e4181b206d541b23851b38f44d7cd 879 878 2011-06-16T15:05:56Z Gsawgwikiadmin 1 wikitext text/x-wiki {| | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |25m |---- |10:35 | |Gaia Alerts overview |STH/LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids with Gaia |Paolo Tanga |25m |---- |12:00 |Gaia |Gaia Spectro Science Alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |14:15 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |16:20 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |16:40 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:40 | |discussion |all |20m |---- |18:00 |end of day 1 | | | |---- | | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- | | | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 |Facilities |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:00 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:20 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:40 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:50 | |The LCOGT network |Yannis Tsapras |20m |---- |12:10 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:10 | |discussion |all |30m |---- |17:40 |end of day 2 | | | |---- | | | | | |---- | | | | | |---- |Friday | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- | | | | | |---- | | | | | |---- | | | | | |---- | | | | | |---- |} 3d9b558e5807dc9872dee92566a08a9b78903bc8 880 879 2011-06-16T15:06:07Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |25m |---- |10:35 | |Gaia Alerts overview |STH/LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids with Gaia |Paolo Tanga |25m |---- |12:00 |Gaia |Gaia Spectro Science Alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |14:15 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |16:20 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |16:40 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:40 | |discussion |all |20m |---- |18:00 |end of day 1 | | | |---- | | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- | | | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 |Facilities |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:00 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:20 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:40 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:50 | |The LCOGT network |Yannis Tsapras |20m |---- |12:10 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:10 | |discussion |all |30m |---- |17:40 |end of day 2 | | | |---- | | | | | |---- | | | | | |---- |Friday | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- | | | | | |---- | | | | | |---- | | | | | |---- | | | | | |---- |} bb9cd7aa347098745094a15e053dd0af9b462bc0 881 880 2011-06-16T15:06:51Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |25m |---- |10:35 | |Gaia Alerts overview |STH/LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids with Gaia |Paolo Tanga |25m |---- |12:00 |Gaia |Gaia Spectro Science Alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |14:15 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |16:20 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |16:40 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:40 | |discussion |all |20m |---- |18:00 |end of day 1 | | | |---- | | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- | | | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 |Facilities |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:00 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:20 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:40 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:50 | |The LCOGT network |Yannis Tsapras |20m |---- |12:10 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |16:10 | |French facilities?? |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:10 | |discussion |all |30m |---- |17:40 |end of day 2 | | | |---- | | | | | |---- |Friday | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 136404ad985595913516bfb3d64aa9af78f57092 882 881 2011-06-16T15:07:47Z Gsawgwikiadmin 1 wikitext text/x-wiki {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |'''Wednesday''' | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |25m |---- |10:35 | |Gaia Alerts overview |STH/LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids with Gaia |Paolo Tanga |25m |---- |12:00 |Gaia |Gaia Spectro Science Alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |14:15 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |16:20 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |16:40 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:40 | |discussion |all |20m |---- |18:00 |end of day 1 | | | |---- | | | | | |---- |19:00 |'''DINNER at St.John's Chop House''' | | | |---- | | | | | |---- |'''Thursday''' | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 |Facilities |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:00 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:20 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:40 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:50 | |The LCOGT network |Yannis Tsapras |20m |---- |12:10 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |16:10 | |French facilities |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:10 | |discussion |all |30m |---- |17:40 |end of day 2 | | | |---- | | | | | |---- |'''Friday''' | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 709a5e1553f2a3de9352283a14b6ed7c0dfadc24 0 138 875 709 2011-06-14T13:38:12Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop stars in late morning on Wednesday 29th of June and will conclude after lunch on Friday, 1st July. The agenda will comprise on presentation of Gaia and Gaia alerts stream, brief outline of scientific topics to which Gaia alerts can contribute, presentations of existing and future transient surveys and follow-up teams and telescopes. The final scope of the agenda, however, will be decided based on the suggested contributions from the participants. The workshop's dinner will take place in St.John's Chop House on Wednesday evening. 9d22dd58bef85de787337efc1572875f804c7bd8 876 875 2011-06-14T14:22:37Z Lukasz 2 wikitext text/x-wiki The workshop stars in late morning on Wednesday 29th of June and will conclude after lunch on Friday, 1st July. The agenda will comprise on presentation of Gaia and Gaia alerts stream, brief outline of scientific topics to which Gaia alerts can contribute, presentations of existing and future transient surveys and follow-up teams and telescopes. The final scope of the agenda, however, will be decided based on the suggested contributions from the participants. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. 0aa436a50d6e94b41008d8cfb9f2e88963e32dcd 883 876 2011-06-16T15:17:00Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |'''Wednesday''' | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |25m |---- |10:35 | |Gaia Alerts overview |STH/LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids with Gaia |Paolo Tanga |25m |---- |12:00 |Gaia |Gaia Spectro Science Alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |14:15 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |16:20 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |16:40 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:40 | |discussion |all |20m |---- |18:00 |end of day 1 | | | |---- | | | | | |---- |19:00 |'''DINNER at St.John's Chop House''' | | | |---- | | | | | |---- |'''Thursday''' | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 |Facilities |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:00 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:20 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:40 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:50 | |The LCOGT network |Yannis Tsapras |20m |---- |12:10 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |16:10 | |Overview of French and other European spectroscopic facilities |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:10 | |discussion |all |30m |---- |17:40 |end of day 2 | | | |---- | | | | | |---- |'''Friday''' | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. c161869294670571a4c4595b0d87a478704e8239 884 883 2011-06-16T15:18:48Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |'''Wednesday''' | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |25m |---- |10:35 | |Gaia Alerts overview |STH/LW |30m |---- |11:05 |coffee | | |30m |---- |11:35 |Gaia |Asteroids with Gaia |Paolo Tanga |25m |---- |12:00 |Gaia |Gaia Spectro Science Alerts |Paola di Mateo |25m |---- |12:25 |lunch | | |90m |---- |13:55 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |14:15 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |14:40 |Science |Variable stars?? |Laurent Eyer |20m |---- |15:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |15:30 | |tea | |30m |---- |16:00 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |16:20 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |16:40 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |17:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:40 | |discussion |all |20m |---- |18:00 |end of day 1 | | | |---- | | | | | |---- |19:00 |'''DINNER at St.John's Chop House''' | | | |---- | | | | | |---- |'''Thursday''' | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 |Facilities |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:00 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:20 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:40 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:00 | |coffee | |30m |---- |11:30 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:50 | |The LCOGT network |Yannis Tsapras |20m |---- |12:10 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:30 | |lunch | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |20m |---- |15:00 | |tea | |30m |---- |15:30 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:50 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |16:10 | |Overview of French and other European spectroscopic facilities |Michel Dennefeld |20m |---- |16:30 | |Italian facilities |Gisella Clementini |20m |---- |16:50 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:10 | |discussion |all |30m |---- |17:40 |end of day 2 | | | |---- | | | | | |---- |'''Friday''' | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. 1157cda9493a2db11e18aa7e4a148e4a03f01479 886 884 2011-06-16T17:12:25Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |11:50 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:10 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:30 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |14:50 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:10 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |16:40 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:00 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:25 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |17:45 |end of day 1 | | | |---- | | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- | | | | | |---- |Thursday | | | | |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |Friday | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- | | | | | |---- |} b84dcdcf9ee53428e2986ddb3c52f5bee50173b2 887 886 2011-06-16T17:19:03Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |11:50 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:10 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:30 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |14:50 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:10 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:20 | |Exotic events?? |Simon Hodgkin?? |20m |---- |16:40 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:00 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:25 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |17:45 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|'''DINNER at St.John's Chop House''' |---- | | | | | |---- |colspan="5"|'''Thursday''' |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 18b879b1806ece668b1d7b4710f8996f41beebb3 890 887 2011-06-20T11:26:22Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="5" | '''''WORKSHOP PHOTO''''' | | |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |14:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |15:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:30 |tea | | |30m |---- |16:00 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |16:20 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:40 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:00 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:20 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:45 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |18:05 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|'''DINNER at St.John's Chop House''' |---- | | | | | |---- |colspan="5"|'''Thursday''' |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 4d413d99a66cc916656a789cab2d5ecf9524d2b6 891 890 2011-06-20T11:26:47Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="4" | '''''WORKSHOP PHOTO''''' |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |14:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |15:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:30 |tea | | |30m |---- |16:00 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |16:20 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:40 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:00 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:20 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:45 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |18:05 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|'''DINNER at St.John's Chop House''' |---- | | | | | |---- |colspan="5"|'''Thursday''' |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 707dfc618547b949355f046fae2b49b8f525ef9a 892 891 2011-06-20T11:26:55Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3" | '''''WORKSHOP PHOTO''''' |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |14:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |15:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:30 |tea | | |30m |---- |16:00 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |16:20 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:40 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:00 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:20 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:45 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |18:05 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|'''DINNER at St.John's Chop House''' |---- | | | | | |---- |colspan="5"|'''Thursday''' |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} 4c5c44e38ccf11347981b5acf0406e723180b6de 893 892 2011-06-20T11:27:09Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="4" | '''''WORKSHOP PHOTO''''' |---- |12:30 |lunch | | |90m |---- |14:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |14:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |15:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:30 |tea | | |30m |---- |16:00 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |16:20 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:40 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:00 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:20 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:45 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |18:05 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|'''DINNER at St.John's Chop House''' |---- | | | | | |---- |colspan="5"|'''Thursday''' |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |PanStarrs &amp; Spectroscopy |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} bc5764b8a57f17a9342c6c003dd9a61cb0261d0a 894 893 2011-06-20T13:30:17Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="4" | '''''WORKSHOP PHOTO''''' |---- |12:30 |lunch | | |90m |---- |14:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |14:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |14:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |15:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |15:30 |tea | | |30m |---- |16:00 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |16:20 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |16:40 | |Exotic events?? |Simon Hodgkin?? |20m |---- |17:00 | |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |17:20 |Facilities |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |25m |---- |17:45 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |18:05 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|'''DINNER at St.John's Chop House''' |---- | | | | | |---- |colspan="5"|'''Thursday''' |---- |09:00 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |09:20 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |09:40 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:00 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |10:20 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |10:40 | |coffee | |30m |---- |11:10 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |11:30 | |The LCOGT network |Yannis Tsapras |20m |---- |11:50 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |12:10 | |lunch | |90m |---- |13:40 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:00 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |14:20 | |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |14:40 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |15:10 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |15:30 | |tea | |30m |---- |16:00 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:20 | |Italian facilities |Gisella Clementini |20m |---- |16:40 | |other facilities (Swiss,Israeli, Polish)??? |??? |20m |---- |17:00 | |discussion |all |30m |---- |17:30 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |Engaging with the public |Gerry Gilmore |20m |---- |09:40 | |What shall we follow today? |Ashish Mahabal |20m |---- |10:00 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |11:00 | |coffee | |30m |---- |11:30 |Discussion |Getting organized |all |60m |---- |12:30 | |lunch | |90m |---- |14:00 |end of day 3 | | | |---- |} f2416b8275c2b0d094228b8ee04770a140242446 896 894 2011-06-21T10:04:31Z Lukasz 2 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|Wednesday |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |WORKSHOP PHOTO | | |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 | |Exotic events?? |Simon Hodgkin?? |20m |---- |18:30 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|DINNER at St.John's Chop House |---- | | | | | |---- |colspan="5"|Thursday |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 |(alternatively: S.Smartt) |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |other facilities (Swiss,Israeli, Polish, Czech)??? |LW/Hudec/? |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|Friday |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} 2199450d1ac9693688d151e0980d7f96698b09b8 897 896 2011-06-22T15:37:59Z Lukasz 2 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote'11, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|Wednesday |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |WORKSHOP PHOTO | | |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 | |Exotic events?? |Simon Hodgkin?? |20m |---- |18:30 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|DINNER at St.John's Chop House |---- | | | | | |---- |colspan="5"|Thursday |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 |(alternatively: Catalina by Ashish) |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |other facilities (Swiss,Israeli, Polish)??? |LW/? |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|Friday |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} f01752ad9f24c1920788b28c660cb3e1c64e5b93 898 897 2011-06-22T15:38:09Z Lukasz 2 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|Wednesday |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |WORKSHOP PHOTO | | |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 | |Exotic events?? |Simon Hodgkin?? |20m |---- |18:30 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"|DINNER at St.John's Chop House |---- | | | | | |---- |colspan="5"|Thursday |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 |(alternatively: Catalina by Ashish) |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |other facilities (Swiss,Israeli, Polish)??? |LW/? |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- | | | | | |---- |colspan="5"|Friday |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} bfd0a10187f10c66b46a2c87388b7472e26602e3 899 898 2011-06-24T11:24:40Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |Wednesday | | | | |---- | | | | | |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |WORKSHOP PHOTO | | |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 | |Exotic events?? |Simon Hodgkin?? |20m |---- |18:30 |end of day 1 | | | |---- | | | | | |---- |19:00 |DINNER at St.John's Chop House | | | |---- | | | | | |---- |Thursday | | | | |---- | | | | | |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 |(alternatively: Catalina) |Exploring Night Sky from the Top of the World. |Utsav Kandel |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |other facilities (Swiss, Israeli, Polish, Austrian)??? |LW? |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- | | | | | |---- |Friday | | | | |---- | | | | | |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} 2b8390acdd1fb5d62647c26995a7fa566a8950e7 900 899 2011-06-27T08:55:26Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"| DINNER at St.John's Chop House |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Real Time Survey |Ashish Mahabal |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} 07b24618e2dd6281fb99ea57c41fe17f22052ff3 901 900 2011-06-27T08:55:51Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"| DINNER at St.John's Chop House |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Real Time Survey |Ashish Mahabal |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} 8cc0077906a93931a21205c461a0c3e2c563f563 0 130 885 671 2011-06-16T16:39:16Z Gsawgwikiadmin 1 wikitext text/x-wiki * Tidal disruption events [http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full_html/2009/08/aa11479-08/aa11479-08.html], [http://arxiv.org/abs/1009.1627] * Lensing by cosmic strings * Optical counterparts to gravitational wave events [https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=1756&version=0] 7f12c57166c51abd006d3ec0bd6f165848421e5f 0 10 895 579 2011-06-20T16:20:26Z Gsawgwikiadmin 1 /* General */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system (from December 2009, not completely up-to-date). Presentation of Gaia and Gaia Alerts with Prezi. <html> <div class="prezi-player"><style type="text/css" media="screen">.prezi-player { width: 550px; } .prezi-player-links { text-align: center; }</style><object id="prezi__3ghuqjeiq6k" name="prezi__3ghuqjeiq6k" classid="clsid:D27CDB6E-AE6D-11cf-96B8-444553540000" width="550" height="400"><param name="movie" value="http://prezi.com/bin/preziloader.swf"/><param name="allowfullscreen" value="true"/><param name="allowscriptaccess" value="always"/><param name="bgcolor" value="#ffffff"/><param name="flashvars" value="prezi_id=_3ghuqjeiq6k&amp;lock_to_path=0&amp;color=ffffff&amp;autoplay=no&amp;autohide_ctrls=0"/><embed id="preziEmbed__3ghuqjeiq6k" name="preziEmbed__3ghuqjeiq6k" src="http://prezi.com/bin/preziloader.swf" type="application/x-shockwave-flash" allowfullscreen="true" allowscriptaccess="always" width="550" height="400" bgcolor="#ffffff" flashvars="prezi_id=_3ghuqjeiq6k&amp;lock_to_path=0&amp;color=ffffff&amp;autoplay=no&amp;autohide_ctrls=0"></embed></object><div class="prezi-player-links"><p><a title="" href="http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/">Around Gaia (Alerts) in 30 questions</a> on <a href="http://prezi.com">Prezi</a></p></div></div> </html> ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** newly acquired G-flux observations, 8-9 measurements separated by 4.4s (per-CCD) ** historical G-flux observations ** mean BP and RP colours ** low-dispersion BP and RP spectrometry (raw,uncalibrated) ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. [[File:gog_sampling.png|200px|left|thumb|Sampling distribution over the whole sky from Gaia simulator]] On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 178256345506d344a74b9e66ad357c6a4c851beb 0 138 902 901 2011-06-27T09:26:53Z Lukasz 2 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"| DINNER at St.John's Chop House |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of French and European spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} 6c316cb4d8d5f14403f65027efe5830d48c647ad 903 902 2011-06-27T10:00:48Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |session |title |name |time (with discussion) |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |coffee | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |lunch | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |tea | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |end of day 1 | | | |---- | | | | | |---- |19:00 |colspan="4"| DINNER at St.John's Chop House |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |coffee | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |lunch | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |tea | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |end of day 2 | | | |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |coffee | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |lunch | | |90m |---- |14:00 |end of day 3 | | | |---- |} 212bb238c3fcc698ffc71c062075e27b71b90049 904 903 2011-06-27T10:04:50Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |''tea'' | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |''lunch'' | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 53a1c59e9a0d4fddd9e1b90e027e3d72cee10ff6 905 904 2011-06-27T10:05:45Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |''tea'' | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |''lunch'' | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 52c5466fc5830e4adaed005758fd5c20644342d1 906 905 2011-06-27T10:06:32Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. <big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |''tea'' | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |''lunch'' | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 4b921a1a423a62bde43dfc1e9ec9ecfe284e7aa9 907 906 2011-06-27T10:06:46Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF. <big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |''tea'' | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |''lunch'' | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 223cde0139ba1619a036c9aaf8e62b89ca8427a6 908 907 2011-06-27T10:07:02Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:25 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |''tea'' | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |''lunch'' | | |90m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} ebdc24122ca30e8e0cc87524d5806bd5a6514f36 909 908 2011-06-27T15:42:50Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 | |''tea'' | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 4e38fb27999d149bac7fe81bf87907baed5a9e5d 910 909 2011-06-27T15:43:26Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 585662a1cc93b8e589abad7667e651c61153c5fe 911 910 2011-06-28T08:59:32Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |Gaia overview |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} d557d7ed212a0b2966f83e42fb9f743178e1e6b6 912 911 2011-06-28T11:25:47Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |Skyalert: Rapid Transients for you and your Robot |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |Prediction of Astrometric Microlensing Events for the Gaia Mission |Svea Proft |20m |---- |17:30 | |The detectability of GRB optical counterparts with Gaia |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |Java Robotic Telescope for Gaia Alert System |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 7b4b2cb42e517b9f989c4b33a7979035c238d747 913 912 2011-06-28T11:27:53Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 8020e8d4db9deb462996c0606130a309fcbd4334 914 913 2011-06-28T11:28:12Z Gsawgwikiadmin 1 wikitext text/x-wiki ''Preliminary agenda as of 27.June 2011'' '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Vasily Belokurov/Wyn Evans |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} e7b1100072e53b9a80dddecd26763673f7cde226 915 914 2011-06-28T11:28:33Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 44e404204d1273401085f43a1adfed22ace199c2 916 915 2011-06-28T15:34:33Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |The La Palma 0.5m Robotic Telescope |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} dac5a367d650e00382d101bc05fbac8b1b4b00ef 917 916 2011-06-28T15:40:22Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 034f84d942288e386a80326971166f1ed4bfadaa 918 917 2011-06-29T08:15:02Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |Gaia Archive Preparations |Nicholas Walton |15m |---- |11:45 | |Gaia Spectro Science Alerts |Paola di Mateo |20m |---- |12:05 | |Asteroids with Gaia |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |What shall we follow today? |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} a10a16ce28798941a51e2bffd3276de15aef7aa7 919 918 2011-06-29T08:20:35Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 5574811d63b5399ae2ca48e37262342c3a21c5fb 920 919 2011-06-29T08:21:03Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |Gaia Alerts overview [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} cc7c2301a2df27a0bffcf31af03e3a1451ec865f 921 920 2011-06-29T08:44:59Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} abf4cc4e29538d29f0f5e0d86bc062d65a0fe5b5 927 921 2011-06-29T12:58:03Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |Variable stars with Gaia |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 125ff3214bc587a3bf291d62dc50a457caa522d9 928 927 2011-06-29T14:03:44Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |Microlensing |Wyn Evans/LW |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 62a35c7b75493afbc4c1a1d2da57469b1a08024a 929 928 2011-06-29T15:04:27Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |Microlensing |Wyn Evans/LW |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |Study of high z Universe with Gaia |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} cc187b14f2de16467ae4a1f0bc0d9fc20a101461 930 929 2011-06-29T15:41:25Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |Microlensing |Wyn Evans/LW |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Hudec_2.pdf Study of high z Universe with Gaia] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} cac9e3215bb786f10e64e324450532520912039d 931 930 2011-06-29T15:42:25Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Hudec_2.pdf Study of high z Universe with Gaia] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 8fd7100bb49026a5439c8e88e779aa01ee553134 932 931 2011-06-30T09:22:02Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Hudec_2.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 58994ebb1ffe4a8ada8fcd3c924a1cadad80f279 933 932 2011-06-30T09:26:06Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |30m |---- |15:10 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |20m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |30m |---- |17:10 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:30 | |discussion |all |30m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} d5efb9a4f9d69a4793cc4fe89166670662eb7974 934 933 2011-06-30T09:32:05Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v2.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |Catalina Realtime Transient Survey (CRTS) |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} c10c840c1ebd37dbec290316629672dd078c7ead 935 934 2011-06-30T09:44:25Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |Gloria - a network of telescopes which can take on some of Gaia alerts |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} b9fcbd57626bfef2b4e0cc60267e4d124cd9cd3a 936 935 2011-06-30T09:47:08Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|WORKSHOP PHOTO |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 53fa424dffb8e14a93f5a42cf692a280bc4b2abe 937 936 2011-06-30T14:21:50Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 4a72166b6bd4fac602b8f9c88cda376b78130cb6 938 937 2011-06-30T14:22:08Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |The LCOGT network |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 34b6eb5e98ac1581e475e53476f2608d3f3e5947 939 938 2011-06-30T15:41:59Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} ad8b06e447474b0fd29b8a0e2baeb16c31511111 940 939 2011-06-30T15:43:31Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |Overview of European and French spectroscopic facilities |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 9623b78e0018cade788930470b2710e0995c8866 941 940 2011-06-30T15:44:10Z Lukasz 2 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |Engaging with the public |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 1fa980e16a43aef1df1f5531f2d3f5d815ea498b 944 941 2011-07-04T16:01:19Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |SNe, overview and follow-up |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes. |Uffe Jorgensen |20m |---- |09:40 | |Galactic transients; linking GAIA alerts with multi-wavelength surveys |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |"Pi of the Sky" - wide field search for optical transients |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |Transients detected in the WASP survey |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |The Liverpool Telescope and Gaia |Iain Steele |20m |---- |14:20 | |STILT (Small Telescopes Installed at LT) instruments |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |Lucky Imaging Astrometric follow-up |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |Italian facilities |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |SAAO facilities and instruments |Patricia Whitelock |20m |---- |09:20 | |The ESO Public spectroscopic survey of the Transient Universe |Stephen Smartt |30m |---- |09:50 | |Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} acc64c86d99c0dbd4c7e161731b74e04f6efae8e 945 944 2011-07-04T16:50:42Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |Iranian National Observatory Project |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 1e522f07cdaf0a75bab1fd36a2f39f138953c250 946 945 2011-07-05T08:50:06Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Similarly to last year we will be recording the presentations to make them available here later on. It will require you to present your talk from our computer. Options available: MS Powerpoint, Keynote, PDF.''' '''<big>Please send your talk to Lukasz Wyrzykowski (wyrzykow@ast.cam.ac.uk)</big>''' ---- Registration will be open from 9am on Wednesday. Coffee will be available. The workshop's dinner will take place in [http://www.stjohnschophouse.co.uk/ St.John's Chop House] on '''Wednesday''' evening. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 1f372e8b49eeb60c888d0f68625c4942f589b113 947 946 2011-07-05T09:14:50Z Lukasz 2 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Microlensing] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 643d40ed11b904605128d1b8e24d03deec20b9c9 948 947 2011-07-07T16:58:46Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} e9f208ebf06ee9178eda831f1bf137a77f8b3c92 949 948 2011-07-07T16:59:19Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] [http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 30c69216a2eb1300c2413c13512238899e9befd6 950 949 2011-07-07T16:59:34Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 88637f7b30aefe235cc71716da69bbf26d3518ad 951 950 2011-07-08T16:34:11Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) |LW |20m |---- |17:20 | |discussion |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} ea090df876e9e6a096e4d368fe81752996f7cf60 0 11 922 710 2011-06-29T10:55:00Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [Users:Lukasz]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 1132539a7c42a904c415750ca71e42cb70ed4905 923 922 2011-06-29T10:55:10Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[Users:Lukasz]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] e5cb834331b231f5e757c5e2f0f158a55c91ccab 924 923 2011-06-29T10:55:17Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 784e83793e15f7157304cf4495d54e4d66379a96 925 924 2011-06-29T10:55:36Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 2cff4e615e03884926a41b304af05510b4c00a99 926 925 2011-06-29T10:55:43Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 765aa4a0f2aff1d7677e8c693e1e60876944f9e9 6 160 942 2011-07-01T08:12:13Z Gaia 3 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 161 943 2011-07-01T08:24:01Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 138 952 951 2011-07-08T16:38:19Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 890e9300a1f1e0cb59d9692c2534fcebabe4d155 953 952 2011-07-08T16:40:28Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 5617ea392102fb3c45abd580d7c34974959b682e 954 953 2011-07-08T16:42:40Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDF and soon the video recording will also be available. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} d2c930fe2a217f11d59aeb66008f3c9fe591e425 955 954 2011-07-08T16:43:55Z Gsawgwikiadmin 1 wikitext text/x-wiki All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdfGaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 15437534f6408b4206b14e79240c905ab1692820 956 955 2011-07-10T11:14:00Z Lukasz 2 wikitext text/x-wiki All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |Whilliam Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 50edf8b07c8d58a61f4e08dc717ccc9c45449a38 966 956 2011-09-07T13:06:42Z Lukasz 2 wikitext text/x-wiki All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 769ab6ad4741075859854c16341da5e9e31ce669 6 162 957 2011-07-15T10:00:56Z Jure.Japelj 24 GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitude. In the case of OAs, the results are given for two different circumburst environments. wikitext text/x-wiki GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitude. In the case of OAs, the results are given for two different circumburst environments. df3d33da7eb4f2a6f0d1426e76d75e863c200ba2 6 163 958 2011-07-15T10:01:53Z Jure.Japelj 24 Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results wikitext text/x-wiki Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results are given for a time of five years. 67a8125accb9ff09a455737514adece534c8ccfd 6 164 959 2011-07-15T10:02:33Z Jure.Japelj 24 Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distrib wikitext text/x-wiki Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distribution of the change in magnitude in the time in which an orphan afterglow is in the field of view. Black distribution corresponds to detection after the peak in a lightcurve while red distribution corresponds to detection before the peak. 58ecafa853da838aff0e7228d60aedfa8bc37f7f 0 73 960 851 2011-07-15T10:13:42Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F5.jpg|thumb|400px|border|right|GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitudes. In the case of OAs, the results are given for two different circumburst environments.]] [[File:F6.jpg|thumb|400px|border|right|Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results are given for a time of five years.]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details on the simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top figure for the case of on-axis and orphan afterglows. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (though it will be smaller for brighter sources [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected GRB optical afterglow detections with Gaia satellite during it's five years of expected operation is of the order of a few tens. Most of the expected detections are of the orphan afterglows, while the possibility of an on-axis afterglow detection is small (less than 10). The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F10.jpg|thumb|400px|border|center|Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distribution of the change in magnitude in the time in which an orphan afterglow is in the field of view. Black distribution corresponds to detection after the peak in a lightcurve while red distribution corresponds to detection before the peak.]] == Simulation references == *J. Japelj, A. Gomboc, Gaia Alerts Workshop 2011, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf presentation] and [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov video recording] of the talk: The detectability of GRB optical counterparts with Gaia *J. Japelj, A. Gomboc, 2011, [http://arxiv.org/abs/1107.2858 arXiv:1107.2858] [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 34ee895cd1cc7840fdddb82ffdf9f18ab1414d52 961 960 2011-07-15T10:14:24Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F5.png|thumb|400px|border|right|GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitudes. In the case of OAs, the results are given for two different circumburst environments.]] [[File:F6.png|thumb|400px|border|right|Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results are given for a time of five years.]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details on the simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top figure for the case of on-axis and orphan afterglows. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, left figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the right. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (though it will be smaller for brighter sources [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected GRB optical afterglow detections with Gaia satellite during it's five years of expected operation is of the order of a few tens. Most of the expected detections are of the orphan afterglows, while the possibility of an on-axis afterglow detection is small (less than 10). The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F10.png|thumb|400px|border|center|Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distribution of the change in magnitude in the time in which an orphan afterglow is in the field of view. Black distribution corresponds to detection after the peak in a lightcurve while red distribution corresponds to detection before the peak.]] == Simulation references == *J. Japelj, A. Gomboc, Gaia Alerts Workshop 2011, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf presentation] and [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov video recording] of the talk: The detectability of GRB optical counterparts with Gaia *J. Japelj, A. Gomboc, 2011, [http://arxiv.org/abs/1107.2858 arXiv:1107.2858] [[User:Jure.Japelj|Jure Japelj]] 18:09, 31 March 2011 (UTC) 1b0bf812b35b0a43d9c182567e553e247754958a 962 961 2011-07-15T10:18:30Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occuring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the lightcurve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow lightcurves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow lightcurves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical lightcurves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F5.png|thumb|400px|border|right|GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitudes. In the case of OAs, the results are given for two different circumburst environments.]] [[File:F6.png|thumb|400px|border|right|Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results are given for a time of five years.]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occuring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details on the simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top figure for the case of on-axis and orphan afterglows. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, right figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the left. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (though it will be smaller for brighter sources [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected GRB optical afterglow detections with Gaia satellite during it's five years of expected operation is of the order of a few tens. Most of the expected detections are of the orphan afterglows, while the possibility of an on-axis afterglow detection is small (less than 10). The problem of afterglow recognition and poor time sampling of the lightcurve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F10.png|thumb|400px|border|center|Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distribution of the change in magnitude in the time in which an orphan afterglow is in the field of view. Black distribution corresponds to detection after the peak in a lightcurve while red distribution corresponds to detection before the peak.]] == Simulation references == *J. Japelj, A. Gomboc, Gaia Alerts Workshop 2011, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf presentation] and [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov video recording] of the talk: The detectability of GRB optical counterparts with Gaia *J. Japelj, A. Gomboc, 2011, [http://arxiv.org/abs/1107.2858 arXiv:1107.2858] [[User:Jure.Japelj|Jure.Japelj]] 11:18, 15 July 2011 (BST) f90e7b0898a9b5fbbca18a16c6727d540ec45854 970 962 2011-09-08T09:34:28Z Jure.Japelj 24 wikitext text/x-wiki === Gamma-Ray Burst Optical Afterglows === [[File:GRB-schematic_lightcurve.png|350px|border|right]] Gamma-ray bursts (GRBs) are extremely energetic, brief and unpredictable explosions occurring on cosmological distances. They represent the most luminous events in the gamma-ray part of the electromagnetic spectrum known in the universe. Often, the prompt gamma-ray emission is followed by an afterglow emitted at longer wavelengths (from X-rays to radio), which can last for several days. Comprehensive review on GRBs and their physics can be found in [http://adsabs.harvard.edu/abs/2004RvMP...76.1143P Piran 2004] or [http://adsabs.harvard.edu/abs/2006RPPh...69.2259M Meszaros 2006]. GRB explosions are believed to be collimated, rather than spherical [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007]. Thus the material, ejected by the explosion, is expanding in the form of a bimodal jet, characterized by an initial half-opening angle [[File:theta.png]]. The shape of the light curve depends on the relative position of the observer's line-of-sight and the axis of the jet cone. We can describe that with an angle [[File:thetaobs.png]] between both directions. We talk about an on-axis GRB and a 'regular' optical afterglow when [[File:theta1.png]]. In the case of [[File:theta2.png]], we can not observe the prompt gamma-ray emission. Due to the beaming effect, we could still observe the so called orphan afterglow (details in [http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] or ). A schematic afterglow light curves for different jet half-opening angles and viewing angles are shown in figure on the right. [[File:kann.png|thumb|350px|border|left|A large sample of regular (on-axis) optical afterglow light curves, corrected for Galactic extinction [http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010].]] A large sample of observed optical light curves of regular 'on-axis' afterglows is shown in figure on the left ([http://adsabs.harvard.edu/abs/2010ApJ...720.1513K Kann et al. 2010]). Observations made by the Swift satellite imply that there are approximately 300 on-axis GRBs per year for which we could observe an optical afterglow. [[File:Color-oa.png|thumb|325px|border|right|Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]..]] Even though orphan afterglows have not been conclusively detected yet, they have been studied a great deal over the last 15 years and various estimations on their detectability have been made ([http://adsabs.harvard.edu/abs/2007RMxAC..27..140G Granot 2007] and references therein). It has been observed, that the color indices (R - I), (V -R) and (B - V) of a sample of observed afterglows are roughly constant in the first 10 days of observation, i.e. their time evolution is negligible. This property could serve as a mean to recognize an afterglow and to distinguish it from other possible sources [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004]. Color-color (B-V vs. V-R) diagram of optical afterglows of long GRBs is shown in figure on the right. All the color indices were corrected for the Galactic reddening. Multiple indices of the same optical afterglow are connected by lines for convenience. Optical afterglows of the ensemble are denoted by open red circles. The mean colors (centroid) of the whole ensemble, including the standard deviations, are marked by the large cross. The outlying optical afterglow of GRB 060218 (closed blue circles) is not included in the calculation of the centroid. The representative reddening paths for E(B-V) = 0.5 mag are shown; they show how much and where the observed data point would move without proper correction (even erroneous correction would thus shift the point only slightly and in predictable direction). Adapted from [http://adsabs.harvard.edu/abs/2001A%26A...377..450S Šimon et al. 2001] [http://adsabs.harvard.edu/abs/2004AIPC..727..487S Šimon et al. 2004] where a detailed information can be found. == Detecting GRBs with Gaia == [[File:F5.png|thumb|400px|border|right|GRB on-axis and OAs detection rate in five years of Gaia's operation as a function of limiting magnitudes. In the case of OAs, the results are given for two different circumburst environments.]] [[File:F6.png|thumb|400px|border|right|Distribution of magnitudes, which are associated with detected afterglows (black), same magnitudes at the time of the first detection (grey) and magnitudes of afterglows detected by the second telescope (red) in the case of on-axis simulation. The results are given for a time of five years.]] In order to predict the number of optical afterglow detections with Gaia in five years of it's time of operation, a simulation was performed. The simulation took into account a scanning law of Gaia, it's field of view, etc. It consists of two parts: one for regular 'on-axis' afterglows and the other for orphan afterglows. In the former the observational data were used to constrain the parameters needed in the simulation (i.e. initial afterglow magnitude distribution, number of afterglows occurring in five years, etc.), while in the latter the parameters were obtained from theoretical predictions. Details on the simulation are given in [[#Simulation references|simulation references]]. Number of detections in respect to limiting magnitude are shown on the the right in the top figure for the case of on-axis and orphan afterglows. The average GRB orphan-afterglow detection rate has been simulated for two different circumburst environments. Bottom, right figure shows initial magnitude distribution of detected on-axis afterglows (black), same distribution at the time of the first detection (gray) and the distribution of detections with the second telescope. Similar plot for orphan afterglows is given in [[#Simulation references|references]]. Since GRB afterglows are initially rapidly fading and they will be observed for 4.4 seconds by each CCD camera, the change of magnitude in that time could in principle be observable. For all detected afterglows in our simulations, we therefore calculated the change of magnitude in 4.4 s, corresponding to observations by two successive CCDs, and also for observations lasting as long as a specific afterglow is in the telescope's field of view. The distribution of the change of magnitude for both cases is shown in the bottom figure on the left. Since the expected photometric error of Gaia at $M_{\rm lim} = 20$ mag will be 10 mmag at best (though it will be smaller for brighter sources [http://www.rssd.esa.int/index.php?project=GAIA&page=index ESA]), the chances of observing the change in magnitudes will be small. To summarize: the number of expected GRB optical afterglow detections with Gaia satellite during it's five years of expected operation is of the order of a few tens. Most of the expected detections are of the orphan afterglows, while the possibility of an on-axis afterglow detection is small (less than 10). The problem of afterglow recognition and poor time sampling of the light curve, in addition to the small number of expected detections, makes the study of GRB optical afterglows with Gaia difficult. On the other hand, since orphan afterglows have not been conclusively detected yet, a possible detection would provide valuable new data. [[File:F10.png|thumb|400px|border|center|Left: Distribution of the change in magnitude in 4.4 s (corresponding to an observation with 2 successive CCDs) (black) and the change of magnitude in the time in which an afterglow is in the entire field of view (red) for the on-axis case. Right: Distribution of the change in magnitude in the time in which an orphan afterglow is in the field of view. Black distribution corresponds to detection after the peak in a light curve while red distribution corresponds to detection before the peak.]] == Simulation references == *J. Japelj, A. Gomboc, Gaia Alerts Workshop 2011, [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf presentation] and [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov video recording] of the talk: The detectability of GRB optical counterparts with Gaia *J. Japelj, A. Gomboc, 2011, [http://arxiv.org/abs/1107.2858 arXiv:1107.2858] [[User:Jure.Japelj|Jure.Japelj]] 11:18, 15 July 2011 (BST) 8f6772c4026bacf976776d4f605f55aaf855eb70 0 17 963 511 2011-08-25T13:44:44Z Lukasz 2 wikitext text/x-wiki == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 7eae327e4050218be275e4789c0268fea247fa81 0 15 964 344 2011-08-29T16:01:20Z Lukasz 2 wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of massive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star * no radio or X-ray counterpart detected * no star visible at that location prior to the outburst on HST archival images. [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. ---- == OT060420 == Very short (~12 min) and bright (~ 5 mag) transient detected by CONCAM all-sky cameras [http://arxiv.org/abs/astro-ph/0607033]. The astronomical nature of the event is disputable, as the detection was made only on two out of three telescopes. One explanation is that the transient was variable. Gaia will be able to detect such transients and also provide per-ccd photometry, every 4 seconds. ---- == Optical transients due to unbound tidal debris == See [http://uk.arxiv.org/abs/0911.5358 Kasen & Ramirez-Ruiz 2009] ---- == Quasar flares (?) == See [http://uk.arxiv.org/abs/1001.2991 Meusinger et al. 2010] ---- == Red giants swallowing planets == Example OGLE-LPV-00861, see Soszynski et al. 2011 and Retter (2006). 80b199860f5037f14d4060b37ffa0613da62db1d 965 964 2011-08-29T16:01:31Z Lukasz 2 /* Red giants swallowing planets */ wikitext text/x-wiki == NGC300-OT == Luminous optical transient was detected in May 2008 in NGC300 by an amateur astronomer B.Monard from South Africa. This object lies in the gap in absolute magnitude between luminous novae and faint supernovae. Nature of the outburst is still debated. Discovery paper by [http://ukads.nottingham.ac.uk/abs/2009ApJ...695L.154B Bond et al. (2008)]. Spitzer/IRS mid-IR spectrum taken 93 days after the maximum ([http://arxiv.org/abs/0907.0230 Prieto et al. 2009]) VLT spectropolarimetric follow-up [http://arxiv.org/abs/0908.0942 Patat et al. 2009]. * maximum absolute brightness: <math>M_V \simeq -12 to -13</math> * detected at brightness <math>V\approx14.5 \textrm{mag}</math> * decay to 20 mag in about 100 days * intermediate between CN and SN * suspected to be a twin with SN 2008S (progenitor: luminous star embedded in circumstellar dust) * probably an explosion of massive (6-10 Msun) carbon-rich AGB/super-AGB or post-AGB star * no radio or X-ray counterpart detected * no star visible at that location prior to the outburst on HST archival images. [[File:NGC300-OT-lightcurve.png]] ---- == Sakurai's Object == V4334 Sgr and similar FG Sge... [[File:SakuraisObjectCMDLMC.png|300px]] Figure from [http://arxiv.org/abs/0907.4090 Spano et al. 2009]. ---- == Luminous Red Novae == New type of novae, introduced in 2007 with detection of M85OT2006-1 transient [http://arxiv.org/abs/astro-ph/0612161 Rau et al. 2006]. Class contains also M31 RV, V4322 Sgr and V838 Mon. See also [http://arxiv.org/abs/0903.0218 Kulkarni et al.2009]. ---- == OT060420 == Very short (~12 min) and bright (~ 5 mag) transient detected by CONCAM all-sky cameras [http://arxiv.org/abs/astro-ph/0607033]. The astronomical nature of the event is disputable, as the detection was made only on two out of three telescopes. One explanation is that the transient was variable. Gaia will be able to detect such transients and also provide per-ccd photometry, every 4 seconds. ---- == Optical transients due to unbound tidal debris == See [http://uk.arxiv.org/abs/0911.5358 Kasen & Ramirez-Ruiz 2009] ---- == Quasar flares (?) == See [http://uk.arxiv.org/abs/1001.2991 Meusinger et al. 2010] ---- == Red giants swallowing planets? == Example OGLE-LPV-00861, see Soszynski et al. 2011 and Retter (2006). 42781919900235448121a27191fba2e55d4aa27f 0 22 967 269 2011-09-07T16:12:17Z Lukasz 2 wikitext text/x-wiki Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 12ab563ef49b19cb3ee563d9bf2419ef5a08e02f 968 967 2011-09-08T09:31:14Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 77b130658bf585922ecca3381947346e1a0023fb 969 968 2011-09-08T09:32:41Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. 2b8cf23ab19f513eff710636d4e373d7bf71d8e1 973 969 2011-09-08T09:38:20Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:FlareGJ3331A-PioftheSky.png|400px]] High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:gj3332.png|thumb|400px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] 6df73f0e7920b16083887678710214cd67511f77 975 973 2011-09-08T09:43:02Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:cn:leo.png|thumb|400px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|400px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] ef0a305d68255a348a7d9a0ed0185a72ad62e1e1 976 975 2011-09-08T09:43:24Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:FlareCNLeo-PioftheSky.png|400px]] Example flare detected by Pi of the Sky project. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008]. [[File:cn_leo.png|thumb|400px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|400px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] fb3ebb241fb11471514bf60ed3089d3537a1f530 977 976 2011-09-08T09:43:52Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:Mdwarf_flare_Gl234AB.png|600px]] Example of flares in Gl234AB (V577 Mon) from [http://ukads.nottingham.ac.uk/abs/1989A%26A...208..208D Doyle et al. 1989] [[File:cn_leo.png|thumb|400px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|400px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] 3ead2604d0a4bd89e306ed30c0ea77e6abd49c6f 978 977 2011-09-08T09:47:18Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|400px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B] Bopp & Moffett 1973.]] [[File:cn_leo.png|thumb|400px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|400px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] 066a8ebfaaeaf0f92730487eded5652fbb731ba2 979 978 2011-09-08T09:48:00Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|400px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:cn_leo.png|thumb|400px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|400px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] 00b8299dc7751bc3e1cf773a8604896812e47ac3 980 979 2011-09-08T09:48:25Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|450px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:cn_leo.png|thumb|450px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] 248e337850094fef94710ee08a35e346acc08c9e 981 980 2011-09-08T09:52:44Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|450px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|450px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] fd634128c35771858d2be7215b3f084aa6f73442 983 981 2011-09-08T09:54:59Z Jure.Japelj 24 /* Light curve examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] 12c13133ad7d052bce7472e72c07d6f4d4993354 985 983 2011-09-08T10:01:35Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] 063b077c80f85076c587e7549788f23326a2ba12 986 985 2011-09-08T10:03:55Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|right|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] \vspace{5.0cm} == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] 40f6a159bccccb59967aefaeb8ec80cc1d92a4e2 987 986 2011-09-08T10:05:27Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] b9a7bb2da47ca398e5303012476fb13a9ae58af0 989 987 2011-09-11T14:01:55Z Jure.Japelj 24 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:m_flare_spectrum.png|thumb|450px|border|right|Spectrum of an M6 dwarf is extremely red. From [http://www.sdss3.org/dr8/data_access.php SDSS DR8]] cb694ecc4ea870ff7adf16608908e33d2d81db0c 990 989 2011-09-11T14:02:25Z Jure.Japelj 24 /* Spectrum examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:m_flare_spectrum.png|thumb|450px|border|right|Spectrum of an M6 dwarf is extremely red. From [http://www.sdss3.org/dr8/data_access.php SDSS DR8]]] 829346e3a88b4f0d54ee73ec25f297d18c1cef22 991 990 2011-09-11T14:02:44Z Jure.Japelj 24 /* Spectrum examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:M_flare_spectrum.png|thumb|450px|border|right|Spectrum of an M6 dwarf is extremely red. From [http://www.sdss3.org/dr8/data_access.php SDSS DR8]]] b9f55449efd21d1e4a360502b7823a43a3c48eec 992 991 2011-09-11T14:03:00Z Jure.Japelj 24 /* Spectrum examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:M_star_spectrum.png|thumb|450px|border|right|Spectrum of an M6 dwarf is extremely red. From [http://www.sdss3.org/dr8/data_access.php SDSS DR8]]] 186a09c48d594eab6d48dfa3f75c1f683abdc79b 993 992 2011-09-11T14:03:34Z Jure.Japelj 24 /* Spectrum examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:M_star_spectrum.png|thumb|450px|border|center|Spectrum of an M6 dwarf is extremely red. From [http://www.sdss3.org/dr8/data_access.php SDSS DR8]]] 7df4dddc40a1bd5ab8115e3b2272d9051b8e8722 6 165 971 2011-09-08T09:35:54Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 166 972 2011-09-08T09:36:09Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 167 974 2011-09-08T09:41:12Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 168 982 2011-09-08T09:54:03Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 169 984 2011-09-08T09:58:57Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 170 988 2011-09-11T13:59:35Z Jure.Japelj 24 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 171 994 2011-09-13T13:17:11Z Sth 6 predictions for SNe alerts with the new scanning law - from Hodgkin & Belokurov. wikitext text/x-wiki predictions for SNe alerts with the new scanning law - from Hodgkin & Belokurov. 1a87afc832aeb1674d814d5760a7925ab6cc8617 0 40 995 669 2011-09-13T13:22:10Z Sth 6 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] Revised numbers can be found here: [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/66/Supernovae_alerts.pdf]. The bottom line is that the total SuperNova catch is more like 19 down to G=19 (2000 before maximum), and about 200 will be brighter than G=16. A figure is reproduced here. == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. d499476e03fc0696bdd5c16cd4b9592077ab6056 997 995 2011-09-13T13:25:30Z Sth 6 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] Revised numbers can be found here: [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/66/Supernovae_alerts.pdf]. The bottom line is that the total SuperNova catch is more like 19 down to G=19 (2000 before maximum), and about 200 will be brighter than G=16. A figure is reproduced here. [file http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/7/74/Gaia_sne.pdf] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. d05f1312a095f477b3851af79a582fa72c0a8f5d 998 997 2011-09-13T13:26:28Z Sth 6 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] Revised numbers can be found here: [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/66/Supernovae_alerts.pdf]. The bottom line is that the total SuperNova catch is more like 19 down to G=19 (2000 before maximum), and about 200 will be brighter than G=16. A figure is reproduced here. [file:http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/7/74/Gaia_sne.pdf] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. 213ae06f1670fd3052aa2058ff543026ecb0ade7 1000 998 2011-09-13T13:28:15Z Sth 6 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] Revised numbers can be found here: [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/66/Supernovae_alerts.pdf]. The bottom line is that the total SuperNova catch is more like 19 down to G=19 (2000 before maximum), and about 200 will be brighter than G=16. A figure is reproduced here. [file:Gaia_sne.png] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. bac651fbd26c950294ef9b00578c984d11ddd8e3 1001 1000 2011-09-13T13:29:14Z Sth 6 wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] Revised numbers can be found here: [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/66/Supernovae_alerts.pdf]. The bottom line is that the total SuperNova catch is more like 19 down to G=19 (2000 before maximum), and about 200 will be brighter than G=16. A figure is reproduced here. [[File:Gaia_sne.png|600px]] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. 2e7abaf8ed4abed2df54d12a1ae47d46784690d0 6 172 996 2011-09-13T13:24:16Z Sth 6 predictions for SNe detections as a function of magnitude wikitext text/x-wiki predictions for SNe detections as a function of magnitude 13aadfb31e88634dbefd6021614cda8c1fa20a81 6 173 999 2011-09-13T13:27:22Z Sth 6 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 40 1002 1001 2011-09-13T13:29:35Z Sth 6 /* Supernova Types and Rates */ wikitext text/x-wiki == Supernova Types and Rates == Numbers based on Belokurov and Evans [http://adsabs.harvard.edu/abs/2003MNRAS.341..569B (2003: MNRAS, 341, 569-576)]. Note that f in the table below is the fraction of all type-II supernovae that are L-type (they suggest using f=0.5). The numbers are derived by taking the Galaxy number counts out to 75 Mpc and extrapolating as D^3. These are combined with supernova event rates compiled from the literature. Although Belokurov and Evans used an old scanning law to make their predictions, the numbers of total events down to G=20 will not change. This magnitude limit corresponds to a distance of 630 Mpc for a type-Ia with an average G-band maximum magnitude of -18.99. {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! Total to G=20 |- | Ia | 48000 |- | Ib | 7000 |- | IIL | 28500*f |- | IIP | 5600*(1-f) |- |} The other piece of information needed is the Luminosity function. Supernova absolute magnitude distributions are also given in Belokurov and Evans. They assume Gaussian distributions of absolute magnitude around maximum brightness as below: {| border="1" cellspacing=0 cellpadding="5" align="center" ! Type ! <math>M_{G}</math> ! <math>\sigma_G</math> |- | 1a | -18.99 | 0.76 |- | 1b/c | -17.75 | 1.29 |- | II-L | -17.63 | 0.88 |- | II-P | -16.44 | 1.23 |- |} Peter Nugent's page with templates for SNe [http://supernova.lbl.gov/~nugent/nugent_templates.html] Revised numbers can be found here: [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/66/Supernovae_alerts.pdf]. The bottom line is that the total SuperNova catch is more like 19 down to G=19 (2000 before maximum), and about 200 will be brighter than G=16. A figure is reproduced here. [[File:Gaia_sne.png|300px]] == Supernovae type Ia == === SDSS-II Supernova Survey (Stripe 82) === Stripe 82 spreads over 300 sq.deg between RA=-60 to RA=60 and Dec=-1.25 to Dec=+1.25. It was monitored by SDSS in 5 filters (''ugriz'') since 1998, but more intensively in 2005 and 2006. Numerous supernovae were found in 2005 season using difference imaging techniques, e.g. [http://ukads.nottingham.ac.uk/abs/2008AJ....135..348S Sako et al. 2008]. [[File:HoltzmanStripe82SNIa.jpg|600px]] From [http://ukads.nottingham.ac.uk/abs/2008AJ....136.2306H Holtzman et al. 2008]. === Rise and fall times of SN Ia === [http://arxiv.org/abs/1001.3428 Hayden et al.2010] studied times of rise and fall of supernovae Ia. They selected a subset of 105 light curves well-observed in both rise and fall portions of the light curves and developed a '2-stretch' fit algorithm which estimates the rise and fall times independently. They found the '''average time from explosion to B-band peak brightness is 17.38 +/- 0.17 days''', but with a spread of rise times which range from 13 days to 23 days. This average rise time is shorter than the 19.5 days found in previous studies. == Supernovae type II == Example of unusual supernova IIn 2008iy [http://uk.arxiv.org/abs/0911.4719 Miller et al. 2009.], which took 400 days to rise. [[File:SN2008iy-phot.png|300px|Photometry of SN2008iy.]] [[File:SN2008iy-spec.png|300px|Spectrometry of SN2008iy. d is the time of discovery.]] For the progenitors of the type IIn the best candidates are Luminous Blue Variables (LBV) [http://xxx.lanl.gov/abs/1011.3484 Dwarkadas (2010)]. == Luminous Red Novae == The class of Luminous Red Novae was established in 2007 by Shrinivas Kulkarni classifying M85 OT2006-1 as LRN. It is disputed if it is a new class or subclass of SN-IIp. * they are fainter than SNe and brighter than novae. * they last over several weeks. * distinctively red in colour, getting redder while fading == Extremely Luminous Supernovae == Type IIn, <math>M_V \approx 22.1~\textrm{mag}</math>, example: 2008fz detected by the Catalina Survey [http://uk.arxiv.org/abs/0908.1990 Drake et al. 2009] == Underluminous Supernovae == Possibly linked with double-degenerate binary systems containing extremely low mass (<0.25 Msol) white dwarfs [http://uk.arxiv.org/abs/1011.3047 Brown et al.(2010)]. 163f10df3c00b690ce97ca684ba152a2bdefb2f2 0 22 1003 993 2011-09-13T15:38:24Z Lukasz 2 /* Spectrum examples */ wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:M_star_spectrum.png|thumb|450px|border|center|Spectrum of an M6 dwarf is extremely red. From [http://cas.sdss.org/dr7/en/tools/chart/navi.asp?ra=194.4769&dec=3.55015 SDSS DR7]]] d3b5a1ede11668bf096dfa7bb96aee4e64d05ef5 1016 1003 2011-10-03T09:46:31Z Lukasz 2 wikitext text/x-wiki === M dwarf flares === Statistical study of M dwarf flares in Stripe 82 is presented in [http://arxiv.org/abs/0906.2030 Kowalski et al. 2009]. Kepler M and K flares are analysed in [http://arxiv.org/abs/1008.0853 Walkowicz et al. 2011]. [[File:Flare_example_Stripe82.png|400px|right]] * Colour range for M-dwarfs (r − i) > 0.53 and (i − z) > 0.3 and (u-r) > 3 * The most flaring are late type M-dwarfs (M4-M6), earlier types (M2-M3) flare half as often as late types and M0-M1 dwarfs flare only 20% as often as late types. * flares are the most pronounced in u-band * around 35% of M-dwarfs are in binary systems - these have bluer u-g. Most single M-dwarfs will have u-g > 1.8 * g - K > 4 - significantly brighter in IR (2MASS cross-match) than Visual. * amplitude in u > 0.7 mag up to 5 mag. * large and small flares possible on the same star * flaring fraction: 0.0108%, i.e. 1 of every 10,000 observation of a M-dwarf in Stripe 82 resulted in a flare * Sloan (5yrs) flaring star probabilities for different types of Mdwarf: M0-M1: 38/35,000; M2-M3: 79/13,000; M4-M6: 119/2120. * 1.3 flares per hour sq.deg with <math>\Delta u > 0.7</math> mag, with slightly more flares towards the galactic plane. [[File:Mflares-rates.png|400px|left]] [[File:FlaresStripe82.png|400px|Ampitude distribution for Stripe82 flares.]] == Light curve examples == [[File:uv_ceti.png|thumb|550px|border|left|High temporal resolution observations of a flare from UV Cet star. From [http://adsabs.harvard.edu/abs/1973ApJ...185..239B Bopp & Moffett 1973.]]] [[File:yzcmi.png|thumb|450px|border|right|The YZ Cmi U-band flare. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010]]] [[File:cn_leo.png|thumb|350px|border|left|Outburst of the flare star CN Leo. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] [[File:gj3332.png|thumb|450px|border|center|High temporal resolution observations of a flare star by Pi of the Sky. From [http://arxiv.org/abs/0810.1179 Sokolowski 2008].]] == Spectrum examples == [[File:yzcmi_spec.png|thumb|450px|border|left|Example of a flare spectrum with an excess of radiation at short wavelengths and pronounced Balmer emission lines. From [http://adsabs.harvard.edu/abs/2010ApJ...714L..98K Kowalski 2010].]] [[File:M_star_spectrum.png|thumb|450px|border|center|Spectrum of an M6 dwarf is extremely red. From [http://cas.sdss.org/dr7/en/tools/chart/navi.asp?ra=194.4769&dec=3.55015 SDSS DR7]]] a2bc55514197463eb3d50693424335d903686532 0 138 1004 966 2011-09-18T14:50:33Z Lukasz 2 wikitext text/x-wiki '''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[File:whitebook2011.pdf|here]].''' ---- All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} c8511041ebbf299c1994efbf807e05ad02f9b4f1 1005 1004 2011-09-18T14:51:11Z Lukasz 2 wikitext text/x-wiki === The White Book === '''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[File:whitebook2011.pdf|here]].''' === Archive and recordings of the talks === All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 8434c6dc463ed507913ab6228efc25d5e0b13ce3 1006 1005 2011-09-18T14:51:25Z Lukasz 2 wikitext text/x-wiki ==== The White Book ==== '''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[File:whitebook2011.pdf|here]].''' ==== Archive and recordings of the talks ==== All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 415480e04c943e22e77b3a73666637646d250630 1008 1006 2011-09-18T14:52:10Z Lukasz 2 wikitext text/x-wiki ==== The White Book ==== '''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[File:whitebook2011.pdf here]].''' ==== Archive and recordings of the talks ==== All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} c6084af155b320b7169a2724a7f43f44cc0bf1d8 1009 1008 2011-09-18T14:52:18Z Lukasz 2 wikitext text/x-wiki ==== The White Book ==== '''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[File:whitebook2011.pdf|here]].''' ==== Archive and recordings of the talks ==== All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 415480e04c943e22e77b3a73666637646d250630 1010 1009 2011-09-18T14:54:11Z Lukasz 2 wikitext text/x-wiki ==== The White Book ==== '''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[Media:whitebook2011.pdf|here]].''' ==== Archive and recordings of the talks ==== All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} cc3ab7a82d0cf0c4590e6905a458156e9de24db7 1011 1010 2011-09-18T14:54:33Z Lukasz 2 wikitext text/x-wiki ==== The White Book ==== <big>'''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[Media:whitebook2011.pdf|here]].'''</big> ==== Archive and recordings of the talks ==== All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 0d016037be51ad43e056a216445c6a6965a44bbc 1012 1011 2011-09-18T14:54:49Z Lukasz 2 wikitext text/x-wiki <center> <big>'''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[Media:whitebook2011.pdf|here]].'''</big> </center> ==== Archive and recordings of the talks ==== All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 283da0dd21b15a6af8e86ef8a647496d50ee0ff2 1013 1012 2011-09-18T14:55:00Z Lukasz 2 wikitext text/x-wiki <center> <big>'''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[Media:whitebook2011.pdf|here]].'''</big> </center> All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} 05370b3574bfde8f0ab9da5fdf6a0a777665b580 1014 1013 2011-09-18T14:55:50Z Lukasz 2 wikitext text/x-wiki == Archive of talks, recording and the White Book == <center> <big>'''The White Book including a brief summary of the talks and the discussions held during the workshop is available [[Media:whitebook2011.pdf|here]].'''</big> </center> All talks are available as PDFs. Video and audio recording is available under '''''rec''''' link. Note, some of the videos are not available or a bit corrupt due to technical issues. ---- {| class="wikitable" | |'''session''' |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="5"|'''Wednesday''' |---- |10:00 | |Welcome |STH/LW |10m |---- |10:10 |Gaia |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/vanLeeuven-SciAlertsWSJune11_v2.pdf Gaia overview] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/vanLeeuven-Gaia.mov rec] |Floor van Leeuven |20m |---- |10:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/hodgkin.pdf Gaia Alerts overview] ([http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/ Prezi on Gaia Alerts]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hodgkin-GaiaScienceAlerts.mov rec] |STH/LW |30m |---- |11:00 |''coffee'' | | |30m |---- |11:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Walton-gap-alerts-jun11.pdf Gaia Archive Preparations] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Walton-GaiaArchivePreparation.mov rec] |Nicholas Walton |15m |---- |11:45 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/dimatteo_spectralalerts.pdf Gaia Spectro Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/diMateo-SpectroscopicAlerts.mov rec] |Paola di Mateo |20m |---- |12:05 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tanga_asteroid_alerts.pdf Asteroids with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tanga-AstrometricAsteroidAlerts.mov rec] |Paolo Tanga |20m |---- |12:35 |''lunch'' | | |95m |---- |14:00 |Special |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110629_GaiaAlertsII_v3.pdf What shall we follow today?] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-What_to_follow.mov rec] |Ashish Mahabal |30m |---- |14:30 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Williams-Skyalert-201106.pdf Skyalert: Rapid Transients for you and your Robot] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Williams-Skyalert.mov rec] |Roy Williams |60m |---- |15:30 |''tea'' | | |30m |---- |16:00 |Science |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Eyer_AlertWGII.pdf Variable stars with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Eyer-VariableStars.mov rec] |Laurent Eyer |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Turatto_2011_Gaia_SNe_v6.pdf (Gaia) Supernovae: overview and follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Turrato-Supernovae.mov rec] |Massimo Turrato |30m |---- |16:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/SveaProft-Microlensing.pdf Prediction of Astrometric Microlensing Events for the Gaia Mission] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Proft-Microlensing.mov rec] |Svea Proft |20m |---- |17:10 | |Microlensing ([http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Evans-Microlensing.pdf Evans], [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/LW-Microlensing_with_Gaia.pdf Wyrzykowski]) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Evans-Wyrzykowski-Microlensing.mov rec] |Wyn Evans/Lukasz Wyrzykowski |20m |---- |17:30 (moved to Thu)) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/gaia_alerts_japelj.pdf The detectability of GRB optical counterparts with Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Japelj-GRBs.mov rec] |Jure Japelj/Andreja Gomboc |20m |---- |17:50 (moved to Thu) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Hudec-Gaia_Alerts2011_Final.pdf Study of high-z Universe with Gaia, Spectroscopic Alerts & Czech Gaia CU7 support by RTs] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Hudec-High-z.mov rec] |Rene Hudec |20m |---- |18:10 |colspan="4"|''end of day 1'' |---- |19:00 |colspan="4"| '''''DINNER at St.John's Chop House''''' |---- |colspan="5"| |---- |colspan="5"|'''Thursday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Seabroke-GBOG.pdf Ground Based Observations for Gaia (GBOG)'s role in Gaia Science Alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Seabroke-GBOG.mov rec] |George Seabroke |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Jorgensen-cambridge2011.pdf Potential follow-up of GAIA alerts from the SONG and MiNDSTEp networks of telescopes.] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Jorgensen-SONG.mov rec] |Uffe Jorgensen |20m |---- |09:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steeghs_GAIA_alerts_Jun11.pdf Galactic transients; linking GAIA alerts with multi-wavelength surveys] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steeghs-CVs.mov rec] |Danny Steeghs |20m |---- |10:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/soldan_jrt.pdf Java Robotic Telescope for Gaia Alert System] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Soldan-JavaRoboticTel.mov rec] |Jan Soldan |20m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Sokolowski-PI.pdf "Pi of the Sky" - wide field search for optical transients] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Sokolowski-PI.mov rec] |Marcin Sokolowski |20m |---- |10:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mankiewcz-Gloria-talk.pdf Gloria - a network of telescopes which can take on some of Gaia alerts] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mankiewicz-Gloria-edited-badrecording.mov rec] |Lech Mankiewicz |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/littlefair_keynote09.pdf The La Palma 0.5m Robotic Telescope] |Stuart Littlefair |20m |---- |11:50 (not presented) | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Wheatley-WASP-Gaia-workshop-june11.pdf Transients detected in the WASP survey] |Peter Wheatley |20m |---- |12:10 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Tsapras-2011_YT_Jun_cambs_gaia_30.06.2011.pdf The LCOGT network] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Tsapras-LCOGT.mov rec] |Yannis Tsapras |20m |---- |12:30 |colspan="3"|[[Media:GaiaAlertsWorkshop-June2011.jpg|WORKSHOP PHOTO]] |5m |---- |12:35 |''lunch'' | | |85m |---- |14:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Steele-LT-Gaia-2011.pdf The Liverpool Telescope and Gaia] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Steele-LiverpoolTel.mov rec] |Iain Steele |20m |---- |14:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mawson-STILT_GAIA_presentation.pdf STILT (Small Telescopes Installed at LT) instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mawson-SkyCamLT.mov rec] |Neil Mawson |20m |---- |14:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/HKhosroshahi-gaia-ioa.pdf Iranian National Observatory Project] |Habib Khosroshahi |20m |---- |15:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mahabal-20110630_GaiaAlertsII-CRTS.pdf Catalina Realtime Transient Survey (CRTS)] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mahabal-Catalina-badrecording.mov rec] |Ashish Mahabal |30m |---- |15:30 |''tea'' | | |30m |---- |16:00 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Mackay-Lucky_AO_Gaia_300611.pdf Lucky Imaging Astrometric follow-up] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Mackay-LuckyImagin.mov rec] |Craig Mackay |20m |---- |16:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Dennefeld-Cambridge_Gaia_June2011.pdf Overview of European and French spectroscopic facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Dennefeld-SpectralFacilities-badrecording.mov rec] |Michel Dennefeld |20m |---- |16:40 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Clementini-Alerts.pdf Italian facilities] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Clementini-ItalianFacilities.mov rec] |Gisella Clementini |20m |---- |17:00 | |Overview of other facilities (Swiss, Israeli, Polish, Austrian) [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Wyrzykowski-OtherFacilities-badrecording.mov rec] |Lukasz Wyrzykowski |20m |---- |17:20 | |Discussion [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion1.mov rec] |all |40m |---- |18:00 |colspan="4"|''end of day 2'' |---- |colspan="5"| |---- |colspan="5"|'''Friday''' |---- |09:00 |Facilities |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Whitelock.pdf SAAO facilities and instruments] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Whitelock-SAAO-nocamera.mov rec] |Patricia Whitelock |20m |---- |09:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Smartt-GAIA-Alerts-June2011.pdf The ESO Public spectroscopic survey of the Transient Universe] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Smartt-ESO-Transient-Survey-nocamera.mov rec] |Stephen Smartt |30m |---- |09:50 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/WThuillot-GREAT-2011.pdf Gaia-FUN-SSO: a ground-based follow-up for Solar System Objects] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Thuillot-GaiaFUN-audio_only.mov rec] |William Thuillot |30m |---- |10:20 | |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Talks/Gilmore-Alerts-outreach.pdf Engaging with the public] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Gilmore-Outreach-audio_only.mov rec] |Gerry Gilmore |20m |---- |10:40 |Discussion |Getting organized [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2011/Movies/Discussion2.mov rec] |all |20m |---- |11:00 |''coffee'' | | |30m |---- |11:30 |Discussion |Getting organized and Summary |all |60m |---- |12:30 |''lunch'' | | |90m |---- |14:00 |colspan="4"|''end of day 3'' |---- |} b2f3d15881d1d1ea3efab893d239a110a6bb251b 6 174 1007 2011-09-18T14:51:56Z Lukasz 2 The Whitebook 2011. wikitext text/x-wiki The Whitebook 2011. 1b38260660b85160405fafca6ddba15f698e9176 1015 1007 2011-09-19T20:10:20Z Lukasz 2 uploaded a new version of &quot;[[File:Whitebook2011.pdf]]&quot; wikitext text/x-wiki The Whitebook 2011. 1b38260660b85160405fafca6ddba15f698e9176 0 11 1017 926 2011-11-03T12:05:57Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] a1a2da1371dd275a4ae57556d207c38106c49869 1018 1017 2011-11-03T12:08:15Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.pdf]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 16967214ed9fd31aad0247430fe5a1762c19f34b 1020 1018 2011-11-03T12:31:03Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] a1a2da1371dd275a4ae57556d207c38106c49869 1022 1020 2011-11-03T12:37:01Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png]] [[File:Example.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 85d70656e503b04644dba3423b96a6f3f5057411 1024 1022 2011-11-03T12:37:58Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] a1a2da1371dd275a4ae57556d207c38106c49869 1025 1024 2011-11-03T12:38:30Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] a5cdab402c2d44e65b1c3c5778fa4c91f50d1139 1031 1025 2011-11-20T13:45:16Z Lukasz 2 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server | Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures. == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] e483fbcd707e7ac161beae19c278e928520860a7 1032 1031 2011-11-20T13:45:29Z Lukasz 2 /* Photometric Calibrations Server */ wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:GaiaAlertsVerificationTimeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] daac722b5ccad6e925e5741c29487f1ea311b543 1050 1032 2012-03-02T10:21:56Z Gsawgwikiadmin 1 wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer@unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini@oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni@oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados@konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] eb9b31b1fa205134faa7117b5d47f900643baf56 6 175 1019 2011-11-03T12:08:22Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 176 1021 2011-11-03T12:36:39Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 177 1023 2011-11-03T12:37:10Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 17 1026 963 2011-11-20T13:37:31Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 2183a986d526307178e1a6a6d80ef1e5cd0bb4e7 1028 1026 2011-11-20T13:42:19Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[Users:wyrzykow | Lukasz Wyrzykowski]] for password. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * ba627c1baf95a46f01961a6aa283bdb8fd1aba48 1029 1028 2011-11-20T13:42:43Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[Users:Lukasz | Lukasz Wyrzykowski]] for password. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 35d3107337f524f42428acd5bdbc7b2f789cf074 1030 1029 2011-11-20T13:43:07Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 5503991f42cbeff3665648b607d82e42437b7c50 1034 1030 2011-11-22T14:43:05Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide also your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 4c2c0054a7704b84305cb574465972aad0f34d34 1035 1034 2011-11-22T14:43:21Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * * 7cb291fad2ad47ccfa6d45c70608c3172306d579 1036 1035 2011-11-22T16:15:53Z Giuseppe.Altavilla 26 /* Current and future instruments suitable for Gaia alerts response */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 314c1e807ea51b35d204d128c46ed1904c1ae4d3 1039 1036 2011-11-29T10:18:58Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 2dce68f03f2bc6c6ff4abacdd69765185d694de4 1040 1039 2011-12-09T14:40:40Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[File:GSAFSManual2011.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 4b17c5b2135c2ca1fd9c6157532ec5e3150e02a1 1042 1040 2011-12-09T14:41:19Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 2dce68f03f2bc6c6ff4abacdd69765185d694de4 1043 1042 2012-01-10T10:50:23Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[File:GSAFSManual2011.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 4b17c5b2135c2ca1fd9c6157532ec5e3150e02a1 1045 1043 2012-01-10T10:51:08Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GSAFSManual2011.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 2dce68f03f2bc6c6ff4abacdd69765185d694de4 6 178 1027 2011-11-20T13:38:50Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1033 1027 2011-11-22T14:42:07Z Lukasz 2 uploaded a new version of &quot;[[File:GSAFSManual2011.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1041 1033 2011-12-09T14:41:06Z Lukasz 2 uploaded a new version of &quot;[[File:GSAFSManual2011.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1044 1041 2012-01-10T10:50:52Z Lukasz 2 uploaded a new version of &quot;[[File:GSAFSManual2011.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 10 1037 895 2011-11-25T17:07:15Z Gsawgwikiadmin 1 wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system (from December 2009, not completely up-to-date). [[Media:AroundGaiaPoster2011.pdf | Poster]] on Gaia Alerts presented at the IAU Symposium #285 in Oxford in September 2011. Presentation of Gaia and Gaia Alerts with Prezi. <html> <div class="prezi-player"><style type="text/css" media="screen">.prezi-player { width: 550px; } .prezi-player-links { text-align: center; }</style><object id="prezi__3ghuqjeiq6k" name="prezi__3ghuqjeiq6k" classid="clsid:D27CDB6E-AE6D-11cf-96B8-444553540000" width="550" height="400"><param name="movie" value="http://prezi.com/bin/preziloader.swf"/><param name="allowfullscreen" value="true"/><param name="allowscriptaccess" value="always"/><param name="bgcolor" value="#ffffff"/><param name="flashvars" value="prezi_id=_3ghuqjeiq6k&amp;lock_to_path=0&amp;color=ffffff&amp;autoplay=no&amp;autohide_ctrls=0"/><embed id="preziEmbed__3ghuqjeiq6k" name="preziEmbed__3ghuqjeiq6k" src="http://prezi.com/bin/preziloader.swf" type="application/x-shockwave-flash" allowfullscreen="true" allowscriptaccess="always" width="550" height="400" bgcolor="#ffffff" flashvars="prezi_id=_3ghuqjeiq6k&amp;lock_to_path=0&amp;color=ffffff&amp;autoplay=no&amp;autohide_ctrls=0"></embed></object><div class="prezi-player-links"><p><a title="" href="http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/">Around Gaia (Alerts) in 30 questions</a> on <a href="http://prezi.com">Prezi</a></p></div></div> </html> ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** newly acquired G-flux observations, 8-9 measurements separated by 4.4s (per-CCD) ** historical G-flux observations ** mean BP and RP colours ** low-dispersion BP and RP spectrometry (raw,uncalibrated) ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. [[File:gog_sampling.png|200px|left|thumb|Sampling distribution over the whole sky from Gaia simulator]] On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 0877e78d875c51eb0519cdd2fd91171a3acd8a50 6 179 1038 2011-11-25T17:08:04Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 24 1046 312 2012-02-02T10:51:05Z Lukasz 2 wikitext text/x-wiki == Science alerts for bright Be stars == Note by Y.Fremat et al. about why and how to do alerts on Be stars: [[File:SciAlertsBeStars.pdf]] == OGLE and MACHO data were studied for Be stars.== * OGLE (LMC,SMC): [http://ukads.nottingham.ac.uk/abs/2005MNRAS.361.1055S Sabogal et al. 2005], [http://ukads.nottingham.ac.uk/abs/2006A%26A...457..949M Mennickent et al. 2006] * OGLE (Bulge): [http://ukads.nottingham.ac.uk/abs/2008A%26A...478..659S Sabogal et al. 2008] 29,000 found in OGLE-II Bulge fields. * MACHO: [http://ukads.nottingham.ac.uk/abs/2002AJ....124.2039K Keller et al. 2002] 1279 found in MACHO LMC data. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] d109d18290e1e88f9904d83a61c04c4332ffb10c 1048 1046 2012-02-02T10:52:17Z Lukasz 2 wikitext text/x-wiki == Science alerts for bright Be stars == Note by Y.Fremat et al. about why and how to do alerts on Be stars: [[Media:SciAlertsBeStars.pdf | PDF]] == OGLE and MACHO data were studied for Be stars.== * OGLE (LMC,SMC): [http://ukads.nottingham.ac.uk/abs/2005MNRAS.361.1055S Sabogal et al. 2005], [http://ukads.nottingham.ac.uk/abs/2006A%26A...457..949M Mennickent et al. 2006] * OGLE (Bulge): [http://ukads.nottingham.ac.uk/abs/2008A%26A...478..659S Sabogal et al. 2008] 29,000 found in OGLE-II Bulge fields. * MACHO: [http://ukads.nottingham.ac.uk/abs/2002AJ....124.2039K Keller et al. 2002] 1279 found in MACHO LMC data. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] aa6171f4e8a2b425c5c594a1de1fc4aa3b5ade74 6 180 1047 2012-02-02T10:51:18Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 181 1049 2012-03-02T10:21:27Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 7 1051 329 2012-03-19T10:53:23Z Gsawgwikiadmin 1 wikitext text/x-wiki ==People contributing to the Science Alerts Working Group== ''Add your name here if you contribute.'' * Institute of Astronomy, Cambridge, UK ** [[user:Lukasz|Lukasz Wyrzykowski]] ** [[user:STH | Simon Hodgkin]] ** [[user:Vasily | Vasily Belokurov]] * Astronomical Institute, AS CR, Czech Republic ** [[Vojtech Simon]] * University of Ljubljana, Slovenia ** Jure Japelj 710a1d25d2fbe7adb98dcb3acecfccf5e45cb7f7 8 3 1052 684 2012-03-19T10:55:19Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2012 ** workshop2012:main|Main Workshop Page ** workshop2012:rationale|Rationale ** workshop2012:agenda|Agenda ** workshop2012:registration|Registration / Participants ** workshop2012:logistics|Logistics * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 68ae4849ad0965e16eb5b7ed256fa40704b50af5 0 1 1053 854 2012-03-19T10:56:50Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>[[Workshop2012:main|Workshop 2012 - Gaia alerts workshop]]</Big> 6-7 September 2012, Bologna, Italy </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 1e51f873e408337681a0f1dacb0be0c086c90ec8 1054 1053 2012-03-19T10:57:06Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>[[Workshop2012:main|Workshop 2012 - Gaia alerts workshop]]</Big> 6-7 September 2012, Bologna, Italy ''details soon'' </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 75a4160080023c0a9699c453c948b3ca556e20f7 1089 1054 2012-03-30T16:39:01Z Gsawgwikiadmin 1 /* Welcome to the web site of the Gaia Science Alerts Working Group! */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> <Big>[[Workshop2012:main|Workshop 2012 - Gaia alerts workshop]]</Big> 6-7 September 2012, Bologna, Italy ''registration open'' </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- fa50ab45c4182dd2938bf44fde866e3e0a698f01 1090 1089 2012-03-30T16:39:13Z Gsawgwikiadmin 1 /* Welcome to the web site of the Gaia Science Alerts Working Group! */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> ''<Big>[[Workshop2012:main|Workshop 2012 - Gaia alerts workshop]]</Big>'' 6-7 September 2012, Bologna, Italy ''registration open'' </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- dc332d5044b8f9a40a1d00f3a058d6d1a7e302c5 1091 1090 2012-03-30T16:39:21Z Gsawgwikiadmin 1 /* Welcome to the web site of the Gaia Science Alerts Working Group! */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big>[[Workshop2012:main|Workshop 2012 - Gaia alerts workshop]]</Big>''' 6-7 September 2012, Bologna, Italy ''registration open'' </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 6e02e60e8beb73adc632b2d598fff75b491f01a4 1092 1091 2012-03-30T16:39:46Z Gsawgwikiadmin 1 /* Welcome to the web site of the Gaia Science Alerts Working Group! */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big>[[Workshop2012:main| Gaia Science Alerts Workshop 2012]]</Big>''' 6-7 September 2012, Bologna, Italy ''registration open'' </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 96c2946a486108d980f384292624d574e53cc51a 0 182 1055 2012-03-23T10:19:59Z Gsawgwikiadmin 1 Created page with "=Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [Media:BOmap.pdf] [[File:..." wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [Media:BOmap.pdf] [[File:BolognaMap.png]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= d1a9495026fdcf832a358720a8d32af4b73833c9 1056 1055 2012-03-23T10:20:07Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf]] [[File:BolognaMap.png]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= 3bdb5f445515ae8cbb2255d4dc1bfdab8446f539 1058 1056 2012-03-23T10:21:10Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf]] [[File:BolognaMap.png| 300px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= 7cf8198cbd7dc9c0439488a6134822e147eb38b8 1059 1058 2012-03-23T10:21:28Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 300px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= 4d25d53f42f4b875847d85bdd632abdac43ba16e 1061 1059 2012-03-23T10:22:07Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= c73dd7d7af66787511a9d1cfd1b921609af2bf2d 1062 1061 2012-03-23T10:27:50Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ 0d8b47effa1241a5d71b8ad8326f901708d153dd 1063 1062 2012-03-23T10:28:41Z Gsawgwikiadmin 1 /* Accommodation */ wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]] 6ed68410554c106d56a399d6092e8f8ee2162bd3 1065 1063 2012-03-23T10:29:18Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ <big>List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]]</big> 0cac1b969033c7e6bce670b99ed2e17fd01accad 1066 1065 2012-03-23T10:30:57Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ <big>List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]]</big> =Lunches and social dinner= The suggested restaurants for lunch are: * 28- ALCE NERO -- Via Petroni 9/b – Tel: 2759196 * 19- CAFFE' UNIVERSITA' -- Via Zamboni 92 – Tel: 244 368 (lunch only) We plan the social dinner on Thursday evening at: * 6 - OSTERIA LA MATTA -- Via Zucchini 9/c -- Tel: 240177 55bb6b54ad0b14db0198a35aac1da3f8bffcbce3 1067 1066 2012-03-23T10:32:52Z Gsawgwikiadmin 1 wikitext text/x-wiki =Travel info= =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ ''(prices valid for December 2011)'' <big>List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]]</big> =Lunches and social dinner= The suggested restaurants for lunch are: * 28- ALCE NERO -- Via Petroni 9/b – Tel: 2759196 * 19- CAFFE' UNIVERSITA' -- Via Zamboni 92 – Tel: 244 368 (lunch only) We plan the social dinner on Thursday evening at: * 6 - OSTERIA LA MATTA -- Via Zucchini 9/c -- Tel: 240177 311cf93ce97a9f67f447d406707ea07e57de7bcd 1068 1067 2012-03-23T10:43:57Z Gsawgwikiadmin 1 wikitext text/x-wiki =Travel info= == By Air == Bologna airport: [http://www.bologna-airport.it/uk/?LN=UK] Direct flights from major European cities, including London (Stansted, Heathrow, Gatwick), Paris, Brussels, Viena, Berlin, Frankfurt (main hub for trans-atlantic flights), Munich, Budapest, Poznan, Lisbon, Barcelona, Madrid, Istanbul. Within Italy direct flights from Rome Fiumicino, Naples, Palermo, Catania. == By Train == Trenitalia [http://www.trenitalia.com] operates very frequent trains from major Italian cities. From Roma Termini to Bologna Centrale: 2h, price from 19 euros. From Milano Centrale to Bologna Centrale: 2h, price from 19 euros From Venezia S.Lucia to Bologna Centrale: 1.5h, price from 19 euros; slow train: 2h, price from 10 euros From Firenze S.M.Novella or Campo Di Marte to Bologna Centrale: 0.5h, price from 19 euros =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ ''(prices valid for December 2011)'' <big>List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]]</big> =Lunches and social dinner= The suggested restaurants for lunch are: * 28- ALCE NERO -- Via Petroni 9/b – Tel: 2759196 * 19- CAFFE' UNIVERSITA' -- Via Zamboni 92 – Tel: 244 368 (lunch only) We plan the social dinner on Thursday evening at: * 6 - OSTERIA LA MATTA -- Via Zucchini 9/c -- Tel: 240177 f12523618bd74f889f9d63da90f618ca4d7de715 1071 1068 2012-03-29T16:53:54Z Gsawgwikiadmin 1 /* Lunches and social dinner */ wikitext text/x-wiki =Travel info= == By Air == Bologna airport: [http://www.bologna-airport.it/uk/?LN=UK] Direct flights from major European cities, including London (Stansted, Heathrow, Gatwick), Paris, Brussels, Viena, Berlin, Frankfurt (main hub for trans-atlantic flights), Munich, Budapest, Poznan, Lisbon, Barcelona, Madrid, Istanbul. Within Italy direct flights from Rome Fiumicino, Naples, Palermo, Catania. == By Train == Trenitalia [http://www.trenitalia.com] operates very frequent trains from major Italian cities. From Roma Termini to Bologna Centrale: 2h, price from 19 euros. From Milano Centrale to Bologna Centrale: 2h, price from 19 euros From Venezia S.Lucia to Bologna Centrale: 1.5h, price from 19 euros; slow train: 2h, price from 10 euros From Firenze S.M.Novella or Campo Di Marte to Bologna Centrale: 0.5h, price from 19 euros =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ ''(prices valid for December 2011)'' <big>List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]]</big> =Lunches and social dinner= The suggested restaurants for lunch are: * 28- ALCE NERO -- Via Petroni 9/b – Tel: 2759196 * 19- CAFFE' UNIVERSITA' -- Via Zamboni 92 – Tel: 244 368 (lunch only) '''We plan the social dinner on Thursday evening at:''' * 6 - OSTERIA LA MATTA -- Via Zucchini 9/c -- Tel: 240177 31717cfe031220b1dbb573b3cc0efb4ab109b870 6 183 1057 2012-03-23T10:20:37Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 184 1060 2012-03-23T10:21:50Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 185 1064 2012-03-23T10:29:04Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 186 1069 2012-03-29T16:45:41Z Gsawgwikiadmin 1 Created page with "== Welcome! == '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Optimisi..." wikitext text/x-wiki == Welcome! == '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Optimising ground-based transient follow-up * Machine learning approaches to the classification of transients * Reviews on current and future transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster2012.jpg|right|300px|]] ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore c0b91b8009caf0aaa4805e684fc18f9784227e1e 1070 1069 2012-03-29T16:45:54Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Optimising ground-based transient follow-up * Machine learning approaches to the classification of transients * Reviews on current and future transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. <!--[[File:Poster2012.jpg|right|300px|]]--> ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore a46c34a6afe9fd9fa8283b9c9649bb391c4fcee3 1096 1070 2012-04-26T16:27:45Z Lukasz 2 wikitext text/x-wiki == Welcome! == '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Optimising ground-based transient follow-up * Machine learning approaches to the classification of transients * Reviews on current and future transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. [[File:Poster2012.jpg|right|300px|]] ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore c0b91b8009caf0aaa4805e684fc18f9784227e1e 1098 1096 2012-04-26T16:28:18Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px|]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Optimising ground-based transient follow-up * Machine learning approaches to the classification of transients * Reviews on current and future transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore 0e2b9f46fafd890f5532cb7de583052f2cc894bb 1099 1098 2012-04-26T16:31:02Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px|]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore d369c2f31e263567655ac1a80c3c767c0f845084 1101 1099 2012-04-26T16:34:22Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px|]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato 127991c94ad5693e35fd44bc0ed8cc6e03ebd5db 0 187 1072 2012-03-29T16:59:51Z Gsawgwikiadmin 1 Created page with " * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with ..." wikitext text/x-wiki * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. 4f05d1ceda93b10f64bda56dbb99b64532909a7b 1073 1072 2012-03-29T17:00:01Z Gsawgwikiadmin 1 wikitext text/x-wiki * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. 8143ac78fcc06576025c62f66577d584b7d14923 1074 1073 2012-03-29T17:00:45Z Gsawgwikiadmin 1 wikitext text/x-wiki First announcement... * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. b313d446aa4d8e006da87c7f94f62f6cb115a020 1093 1074 2012-03-30T16:40:49Z Gsawgwikiadmin 1 wikitext text/x-wiki The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested. Therefore, the first alerts will need to be verified with an extensive programme of dedicated follow-up observations. Thorough and robust classification requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. ---- The main goals of the meeting: * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. f7c60e42aa0130b774b019bcc88c35a92ebfb094 1094 1093 2012-03-30T16:41:15Z Gsawgwikiadmin 1 wikitext text/x-wiki === Workshop announcement === The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested. Therefore, the first alerts will need to be verified with an extensive programme of dedicated follow-up observations. Thorough and robust classification requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. ---- === The main goals of the meeting === * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. a59045a801af17969ffdae9b7b25ca74682876a4 0 188 1075 2012-03-29T17:03:14Z Gsawgwikiadmin 1 Created page with "==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Registration will close on the 15t..." wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Registration will close on the 15th of August 2012.''' a6bbe0226ece963b3d5c83e7051031ee20e70961 1081 1075 2012-03-30T10:43:32Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. ''Please note that due to lack of funding this year, there will be a 45 euro workshop fee, payable at the arrival to the workshop.'' '''Registration will close on the 15th of August 2012.''' 2d2822cba5f0ca85b38eb86cb9630e8cc0cb2734 1082 1081 2012-03-30T10:43:42Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''''Please note that due to lack of funding this year, there will be a 45 euro workshop fee, payable at the arrival to the workshop.''''' '''Registration will close on the 15th of August 2012.''' f19cf027438ee9c7fa94038801e4b409f19f41e6 1083 1082 2012-03-30T10:43:55Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a 45 euro workshop fee, payable at the arrival to the workshop.''' ''Registration will close on the 15th of August 2012.'' 67c6cbdc692c09cebeb3da432bf056944c516281 1084 1083 2012-03-30T10:44:19Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>45 euro</big> workshop fee, payable at the arrival to the workshop.''' ''Registration will close on the 15th of August 2012.'' b269648f29c8a8d6e738168063e7af253a78defb 1085 1084 2012-03-30T10:45:18Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' 5c5fb6188a87fc084b11ad6959796147a3527993 1086 1085 2012-03-30T10:46:53Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- Registration form is available [[Workshop2012:registrationform | here]]. 25931f652d846fcbe6029aa8d5fecfc1f58bd4c9 1087 1086 2012-03-30T10:47:07Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>Registration form is available [[Workshop2012:registrationform | here]].</big> f82d3a8ec256c589caa1c29ed4205d9e3bb2ede7 1088 1087 2012-03-30T10:47:32Z Gsawgwikiadmin 1 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> de4399538fc086dac652bf512236e53f21e81cd4 0 189 1076 2012-03-29T17:13:54Z Gsawgwikiadmin 1 Created page with "== Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast...." wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsawg@ast.cam.ac.uk'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- ''' Arrival/departure''' Please provide us with the dates of your arrival/departure to/from Cambridge: {| |- | Arrival: | {{#input:type=text|name=arrival|value=28/06/2011}} | Departure: | {{#input:type=text|name=departure|value=01/07/2011}} |} ---- '''Accommodation''' ''We have booked a set of single and double rooms in the nearby Churchill College. If you are interested in this accommodation you will be asked to pay for your stay in advance.'' ''Alternatively you can book a room in one of the hotels or B&Bs in Cambridge. Check the Logistics page.'' {| |- | I would like to book a room in the Churchill College from 28/06 to 01/07 (contact us if you need to book for other dates) | {{#input:type=select|name=accom_churchill| |- *Please select *yes *no, I'll find accommodation myself}} |} {| | Room type: | {{#input:type=select|name=accom_roomtype| *single at 58 GBP per night *twin at 72 GBP per night}} |} ---- '''Workshop's Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 30th''''' ''in the St.John's Chop House restaurant.'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Financial support''' ''We are able to provide very limited support for travel or accommodation, mainly for students.'' {| |- | I would like to apply for the support: | {{#input:type=select|name=support| *no *yes}} |} ''Brief (<250 words) justification of your need for financial support. Please include amount of money you would like to apply for (in pounds).'' {{#input:type=textarea|name=justification|rows=3|cols=100|style=width:auto}} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 5ec5df94042ca7f9af8c53342d801c0b40f91a24 1077 1076 2012-03-30T09:57:40Z Gsawgwikiadmin 1 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2012@gmail.com'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 6th''''' ''in the Osteria la Matta'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 584163fcadbf1cb93fe84d8b5c6fc57b700c3011 0 190 1078 2012-03-30T10:08:06Z Gsawgwikiadmin 1 Created page with "'''Thursday, September 6th''' First day Social dinner '''Friday, September 7th''' Second day" wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner '''Friday, September 7th''' Second day 45fab847ddfdd9f0ccb66df2359883ed71557d68 1079 1078 2012-03-30T10:09:27Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner at Osteria la Matta -- Via Zucchini 9/c '''Friday, September 7th''' Second day f462b21f91caae71ec0018096e4fd9f9c6c72ed9 1080 1079 2012-03-30T10:09:34Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day 8f5fdbf567a1fa83208f34b5fe5b35ae3ae395bc 1095 1080 2012-04-12T08:45:35Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Building the network, discussion on further steps The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 5a2e97c95dbd5c82e82d6903cd63c639e31be594 1100 1095 2012-04-26T16:32:10Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Building the network, discussion on further steps The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 5649c86add17e4c2d63b3f4a0aa3b30ecafca2db 6 191 1097 2012-04-26T16:27:59Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 130 1102 885 2012-05-22T16:43:21Z Lukasz 2 wikitext text/x-wiki * Tidal disruption events [http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full_html/2009/08/aa11479-08/aa11479-08.html], [http://arxiv.org/abs/1009.1627], [http://www.nature.com/nature/journal/vaop/ncurrent/full/nature10990.html] * Lensing by cosmic strings * Optical counterparts to gravitational wave events [https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=1756&version=0] 0440d67888ffae136c0c213a7b90d2c6f6252896 1103 1102 2012-05-22T16:43:29Z Lukasz 2 wikitext text/x-wiki * Tidal disruption events [http://www.aanda.org/index.php?option=com_article&access=standard&Itemid=129&url=/articles/aa/full_html/2009/08/aa11479-08/aa11479-08.html], [http://arxiv.org/abs/1009.1627], [http://www.nature.com/nature/journal/vaop/ncurrent/full/nature10990.html] * Lensing by cosmic strings * Optical counterparts to gravitational wave events [https://dcc.ligo.org/cgi-bin/DocDB/ShowDocument?docid=1756&version=0] 24531984fce2569b83fd5d8f1fe7b934f8accce6 0 187 1104 1094 2012-05-29T13:03:56Z Lukasz 2 wikitext text/x-wiki === Workshop announcement === [[Full first announcement]] The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested. Therefore, the first alerts will need to be verified with an extensive programme of dedicated follow-up observations. Thorough and robust classification requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. ---- === The main goals of the meeting === * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. 636109986b489e8774fa0c88993134aacd0c5b4f 1106 1104 2012-05-29T13:06:04Z Lukasz 2 wikitext text/x-wiki === Workshop announcement === [[Full first announcement]] of March 31st 2012 The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested. Therefore, the first alerts will need to be verified with an extensive programme of dedicated follow-up observations. Thorough and robust classification requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. ---- === The main goals of the meeting === * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. 0f9fc4246a471448350c003f3eb86a69e777d0af 1111 1106 2012-06-11T11:50:41Z Lukasz 2 wikitext text/x-wiki === Workshop announcement === [[Full first announcement]] of March 31st 2012 [[Full second announcement]] of June 11th 2012 The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested. Therefore, the first alerts will need to be verified with an extensive programme of dedicated follow-up observations. Thorough and robust classification requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. ---- === The main goals of the meeting === * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. 95dcb793466d49a343cdbddf620758fd004e6e85 1116 1111 2012-06-11T11:58:00Z Lukasz 2 wikitext text/x-wiki === Workshop announcements=== [[Full first announcement]] of March 31st 2012 [[Full second announcement]] of June 11th 2012 === Rationale === The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested and cross-matched with detections made by other surveys, both optical and in other wavelengths. Thorough and robust classification of transients requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. ---- === The main goals of the meeting === * '''Optimising ground-based transient follow-up''' It can be shown that for any given transient, there exists a wide-range of follow-up observations that could be made, with differing degrees of effectiveness for improving classification. We will consider the general question ''what should we do next?'', and investigate the dependence of the answer to this question on (i) the nature of the event, (ii) the availability and quality of measured data (photometry, astrometry, spectroscopy), (iii) the telescope and instrumentation available to the observer. This workshop session will look at the follow-up teams experiences with the CRTS and other surveys data. * '''Machine learning approaches to the classification of transient data'''. Classification of transients is a unique problem for computational astrophysics. In this part of the workshop we will discuss state-of-the-art techniques for transient classification, including: Gaussian Mixtures, Self-Organizing Maps, Random Forest, Neural Networks, naive Bayes and so on. A workshop session will focus on the application of these techniques to the transients surveys data stream, and comparison to the Gaia data stream. * '''Expanding the follow-up community''' There are a large number of telescopes and observers around the globe, both suitable and interested in taking part in the follow-up of the Gaia alerts. The list includes professional astronomers, as well as skilled,hard-working, well-equipped and well-organised amateur astronomers who would love to work closely with the Gaia mission. One of the main goals of our meeting is to identify new potential partners for the alerts follow-up and discuss common practises for the follow-up process, with an emphasis on the verification of the Gaia alerts. As an outcome of this we hope to prepare an agreed version of the ''Memorandum of Understanding'', to be signed between the Gaia Science Alerts team and partners. This will cover all issues related with the data dissemination, processing and usage policy. An additional deliverable will be an evolving web site describing recommended follow-up procedures, providing detailed instructions on how to get involved, how to observe, how to share data, and instructing the astronomers how and who to credit. 9959e9026fa1b4de086e355e70001a87e444ed8e 0 192 1105 2012-05-29T13:05:35Z Lukasz 2 Created page with "Dear Colleagues, The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST)..." wikitext text/x-wiki Dear Colleagues, The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost. It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested. Therefore, the first alerts will need to be verified with an extensive programme of dedicated follow-up observations. Thorough and robust classification requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. Workshop will take place on 6-7 September 2012 in the old university of Bologna in Italy. Further details and registration is available here: http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Workshop2012:main Best regards and hope to see you in Bologna! Lukasz Wyrzykowski on behalf of the Workshop Organizing Committee ----------------------------------------------------- Gaia Science Alerts Workshop 2012 6-7 September 2012, Bologna, Italy http://www.ast.cam.ac.uk/ioa/research/gsawg email: gsaw2012@gmail.com bf118de62b71313d81d592b364a3d711e3f35524 0 188 1107 1088 2012-05-29T13:08:03Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: * Eran Ofek * Massimo Turatto * Minia Manteiga Outeiro * Petr Kubanek 26d49f077d77f3ac6ee81c94397c8e119de56945 1109 1107 2012-05-30T08:48:44Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: * Eran Ofek * Massimo Turatto * Minia Manteiga Outeiro * Petr Kubanek * Gianluca M Guidi * Vladimir Lipunov 0f26fecf7b920a23ea80d113c43b363c1224e3dd 1117 1109 2012-06-11T16:00:04Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: * Eran Ofek * Massimo Turatto * Minia Manteiga Outeiro * Petr Kubanek * Gianluca M Guidi * Vladimir Lipunov * Michel Dennefeld 2a4994e4b4ed8818cac4766e6db45c0071234a22 1118 1117 2012-06-11T16:17:28Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld 7532f5d01790ba54cccda28c037515ed9fedd7c5 1122 1118 2012-06-13T13:19:16Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore 745160f1d72595fce8c7555025d202f477f9082e 1129 1122 2012-06-20T12:01:48Z Lukasz 2 /* Registration */ wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele 9453a994466eee068b135b483209d2733134c18a 1135 1129 2012-06-26T10:45:31Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi a8af0772d5f4f9636d085144f5ccaf3f650b6122 1136 1135 2012-06-29T09:56:46Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''Please note that due to lack of funding this year, there will be a <big>50 euro</big> workshop fee, payable at the arrival to the workshop. This will cover the local costs, including coffee breaks. ''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti c164be001915d172184704f206e224461b756621 1137 1136 2012-07-11T12:52:39Z Lukasz 2 /* Registration */ wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti 3ce548f9c4c14c4f5920f1a6b9a51a1a0e94787c 1151 1137 2012-07-17T21:13:42Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres c2f01f5788025bbd76283c520296bcc9cb7414b7 0 11 1108 1050 2012-05-29T13:35:51Z Lukasz 2 /* Preliminary list of telescopes and people involved */ wikitext text/x-wiki The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 8d2c22050c4e8a184a594a7f6d19f3b6addb4769 0 186 1110 1101 2012-06-11T11:36:54Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px|]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato d3e0a68f60ca2b121cb02db964ec4dbb47ea1042 1119 1110 2012-06-12T13:11:11Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px|]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato 2457ca62e0346814e526c482f8d9ae6ab4cf4005 1141 1119 2012-07-16T09:45:22Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px|poster2012page]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato c4bca813fd46579782cc91ce12126e75b0af5fd2 1142 1141 2012-07-16T09:45:36Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] <!--* [[workshop2012:poster|Workshop's poster for download]]--> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato f68dc79cc06b8d373783abc345eb68d94eddfe88 1143 1142 2012-07-16T09:46:03Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato bfbabd06de473d6aa41a40809a19c7505cc9aaeb 0 193 1112 2012-06-11T11:51:10Z Lukasz 2 Created page with "Dear Colleagues, We would like to invite you to the 3rd Gaia Science Alerts Workshop, which will take place in Bologna, Italy on 6-7 September 2012.  The transient sky has nev..." wikitext text/x-wiki Dear Colleagues, We would like to invite you to the 3rd Gaia Science Alerts Workshop, which will take place in Bologna, Italy on 6-7 September 2012.  The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested and cross-matched with detections made by other surveys, both optical and in other wavelengths. Thorough and robust classification of transients requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. Among the participants: - Ashish Mahabal, CRTS, Caltech, USA - Robert Quimby, PTF, Japan - Eran Ofek, PTF, Israel - Petr Kubanek, RTS2, BOOTES, Czech Republic - Timo Prusti, Gaia, ESA - Massimo Turatto, Padova, Italy - Patrick Tisserand, Skymapper, Canberra, Australia - Peter Jonker, LOFAR (radio transients), SRON, The Neatherlands - Vladimir Lipunov, MASTER-net, Moscow, Russia - Laurent Eyer, Gaia, Geneva, Switzerland - Gianluca M Guidi, Virgo Collaboration (gravitational wave observatory), Urbino, Italy - Pietro Antonioli, SNEWS (neutrino observatories), Bologna, Italy Details and registration: http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Workshop2012:main Best regards, Lukasz Wyrzykowski on behalf of the Workshop Organizing Committee ----------------------------------------------------- Gaia Science Alerts Workshop 2012 6-7 September 2012, Bologna, Italy http://www.ast.cam.ac.uk/ioa/research/gsawg email: gsaw2012@gmail.com 6278271162b577a5aa6e51aea9c3e2e535d2a735 1113 1112 2012-06-11T11:51:43Z Lukasz 2 wikitext text/x-wiki Dear Colleagues, We would like to invite you to the 3rd Gaia Science Alerts Workshop, which will take place in Bologna, Italy on 6-7 September 2012.  The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested and cross-matched with detections made by other surveys, both optical and in other wavelengths. Thorough and robust classification of transients requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. Among the participants: - Ashish Mahabal, CRTS, Caltech, USA - Robert Quimby, PTF, Japan - Eran Ofek, PTF, Israel - Petr Kubanek, RTS2, BOOTES, Czech Republic - Timo Prusti, Gaia, ESA - Massimo Turatto, Padova, Italy - Patrick Tisserand, Skymapper, Canberra, Australia - Peter Jonker, LOFAR (radio transients), SRON, The Neatherlands - Vladimir Lipunov, MASTER-net, Moscow, Russia - Laurent Eyer, Gaia, Geneva, Switzerland - Gianluca M Guidi, Virgo Collaboration (gravitational wave observatory), Urbino, Italy - Pietro Antonioli, SNEWS (neutrino observatories), Bologna, Italy Details and registration: http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Workshop2012:main Best regards, Lukasz Wyrzykowski on behalf of the Workshop Organizing Committee ----------------------------------------------------- Gaia Science Alerts Workshop 2012 6-7 September 2012, Bologna, Italy http://www.ast.cam.ac.uk/ioa/research/gsawg email: gsaw2012@gmail.com 4abf97a45b4803e18005e4aeb394d09c54c77656 1114 1113 2012-06-11T11:51:52Z Lukasz 2 wikitext text/x-wiki Dear Colleagues, We would like to invite you to the 3rd Gaia Science Alerts Workshop, which will take place in Bologna, Italy on 6-7 September 2012.  The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested and cross-matched with detections made by other surveys, both optical and in other wavelengths. Thorough and robust classification of transients requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. Among the participants: - Ashish Mahabal, CRTS, Caltech, USA - Robert Quimby, PTF, Japan - Eran Ofek, PTF, Israel - Petr Kubanek, RTS2, BOOTES, Czech Republic - Timo Prusti, Gaia, ESA - Massimo Turatto, Padova, Italy - Patrick Tisserand, Skymapper, Canberra, Australia - Peter Jonker, LOFAR (radio transients), SRON, The Neatherlands - Vladimir Lipunov, MASTER-net, Moscow, Russia - Laurent Eyer, Gaia, Geneva, Switzerland - Gianluca M Guidi, Virgo Collaboration (gravitational wave observatory), Urbino, Italy - Pietro Antonioli, SNEWS (neutrino observatories), Bologna, Italy ---- Details and registration: http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Workshop2012:main Best regards, Lukasz Wyrzykowski on behalf of the Workshop Organizing Committee ----------------------------------------------------- Gaia Science Alerts Workshop 2012 6-7 September 2012, Bologna, Italy http://www.ast.cam.ac.uk/ioa/research/gsawg email: gsaw2012@gmail.com dc15ce8ea6ad485257f795537d8b92c26a0a3871 1115 1114 2012-06-11T11:52:29Z Lukasz 2 wikitext text/x-wiki Dear Colleagues, We would like to invite you to the 3rd Gaia Science Alerts Workshop, which will take place in Bologna, Italy on 6-7 September 2012.  The transient sky has never been more exciting. Numerous current and near-future large-scale surveys (PanStarrs, PTF, SkyMapper, Gaia, SWIFT, OGLE, LOFAR, LSST) are promising vast numbers of new, transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to Supernovae and orphan Gamma Ray Bursts. However without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost.  It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. The Gaia Photometric Science Alerts team, is responsible for generating alerts on transient and anomalous events detected in the data stream of the Gaia satellite  - cornerstone ESA mission scheduled for launch in August 2013. The alerts will become public immediately, and to assure the complex data processing pipeline produces reliable and robust alerts, they need to be thoroughly tested and cross-matched with detections made by other surveys, both optical and in other wavelengths. Thorough and robust classification of transients requires a dedicated network of telescopes and a well-organised team. Now, with the Gaia launch so close, we are approaching a crucial point in time. We need to organise our teams, choose instruments and telescopes, construct observing proposals, and prepare the community for the influx of Gaia alerts. During the first two Gaia Science Alerts workshops we have addressed the requirements for the ground-based verification of alerts and their follow-up. We have established the foundations of the collaborative network of telescopes and scientists willing to get involved in the transients follow-up and Gaia alerts verification. In the third workshop this summer we will present and discuss the early-stage tests performed by our partners based on alerts generated by the Catalina Real-Time Transient Survey (CRTS) and other surveys. We will also continue building and extending the network with new partners. One of the main issues related with the follow-up of transients is their robust and rapid classification at the survey level and then  evolving classification with the additional follow-up data. We will concentrate on this subject during the third workshop and present current techniques and methods of transient classification presented by experts in the field and astronomers applying the techniques to their data. Among the participants: * Ashish Mahabal, CRTS, Caltech, USA * Robert Quimby, PTF, Japan * Eran Ofek, PTF, Israel * Petr Kubanek, RTS2, BOOTES, Czech Republic * Timo Prusti, Gaia, ESA * Massimo Turatto, Padova, Italy * Patrick Tisserand, Skymapper, Canberra, Australia * Peter Jonker, LOFAR (radio transients), SRON, The Neatherlands * Vladimir Lipunov, MASTER-net, Moscow, Russia * Laurent Eyer, Gaia, Geneva, Switzerland * Gianluca M Guidi, Virgo Collaboration (gravitational wave observatory), Urbino, Italy * Pietro Antonioli, SNEWS (neutrino observatories), Bologna, Italy Details and registration: http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Workshop2012:main Best regards, Lukasz Wyrzykowski on behalf of the Workshop Organizing Committee ----------------------------------------------------- Gaia Science Alerts Workshop 2012 6-7 September 2012, Bologna, Italy http://www.ast.cam.ac.uk/ioa/research/gsawg email: gsaw2012@gmail.com 69ff391334ba405fce03e1b4e6841d071e46711b 0 190 1120 1100 2012-06-12T13:58:13Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Discussing the details of the operation during the verification phase, including Memorandums of Understanding * Presentation of tools for coordinated follow-up observations of transients The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. b0d8b576ca828a38a708487a2797c0b7831772ff 1121 1120 2012-06-12T13:58:27Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Discussing the details of the operation during the verification phase, including Memorandums of Understanding * Presentation of tools for coordinated follow-up observations of transients The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 2ec8c9fda8e96d8987b2af889c72bdd4b120f4cd 6 181 1123 1049 2012-06-14T14:22:18Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1124 1123 2012-06-14T14:24:24Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 51 1125 284 2012-06-18T11:21:25Z Lukasz 2 wikitext text/x-wiki == R Corona Borealis stars == Clayton's review on RCB stars: [http://xxx.lanl.gov/abs/1206.3448] [[File:figure_rcrb_mag.png|300px|right|thumb|Example of RCrB star in the LMC as seen by OGLE-II]] Only around 50 known in the Galaxy and Magellanic Clouds. They are rare type of evolved carbon-rich and hydrogen-deficient evolved F and G supergiants that are thought to result from the merger of two white dwarfs, called the Double Degenerate (DD) scenario. This scenario is also studied in context of SN Ia explosions, therefore better understanding of RCrB stars is crucial. [http://arxiv.org/abs/0905.3224 Tisserand et al. 2009]. Characteristics: * sudden and non-periodic drops in magnitude * drops by up to 9 magnitudes * some small variation in the baseline * the "dark" stage can last from days to years * recovers slowly to the baseline * fading rate: 0.04 mag/day * absolute magnitude range: M_V=-5.2 to -3.4 mag * 0 < V-I < 2 * near-infrared excess: between 0 and 3 in J-H and H-K [[File:RCRB-nearIR.png|700px]] == DY Persei == [[File:DYPer.png|300px|right|thumb|Example OGLE light curve of DY Per-type candidate]] These are another Carbon stars. Their drops in magnitude are much smaller than in RCrBs and seem to be periodical (P~1000d). * their distributions match those of typical carbon stars (type N) * fading rate: 0.01 mag/day * absolute magnitude range: M_V=-3 to -1.8 mag * V-I > 1.5 6263f5a68d1ea11933dfd6714595d6beee1ef033 0 17 1126 1045 2012-06-20T11:05:57Z Lukasz 2 /* Gaia Science Alerts Follow-up Server */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[File:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 26c474148f9cd9cba280d2106947336e9d4da431 1128 1126 2012-06-20T11:06:55Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 549ce5959064186b84029e1afc59241701aa4a8c 1130 1128 2012-06-20T14:38:55Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [[http://nova.astrometry.net Astrometry.net]] - online service providing astrometric WCS solution for any image * [[http://www.astromatic.net Astromatic.net]] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 48ecf23a5854f9b9865d13194cebbc5c3fd55bc5 1131 1130 2012-06-20T14:39:13Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 7e2f990582fc99ef4af20e38b8407256f4ca11c9 6 194 1127 2012-06-20T11:06:19Z Lukasz 2 version of June 2012. wikitext text/x-wiki version of June 2012. a88ad5fcc354459febd089042467faaff874658b 0 24 1132 1048 2012-06-22T16:21:45Z Lukasz 2 /* Science alerts for bright Be stars */ wikitext text/x-wiki == Science alerts for bright Be stars == Note by Y.Fremat et al. about why and how to do alerts on Be stars: [[File:SciAlertsBeStars.pdf | PDF]] == OGLE and MACHO data were studied for Be stars.== * OGLE (LMC,SMC): [http://ukads.nottingham.ac.uk/abs/2005MNRAS.361.1055S Sabogal et al. 2005], [http://ukads.nottingham.ac.uk/abs/2006A%26A...457..949M Mennickent et al. 2006] * OGLE (Bulge): [http://ukads.nottingham.ac.uk/abs/2008A%26A...478..659S Sabogal et al. 2008] 29,000 found in OGLE-II Bulge fields. * MACHO: [http://ukads.nottingham.ac.uk/abs/2002AJ....124.2039K Keller et al. 2002] 1279 found in MACHO LMC data. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] 8d13e696143bd25bfa3ffb01b32daadfd0ecddb9 1134 1132 2012-06-22T16:22:23Z Lukasz 2 /* Science alerts for bright Be stars */ wikitext text/x-wiki == Science alerts for bright Be stars == Note by Y.Fremat et al. about why and how to do alerts on Be stars: [[Media:SciAlertsBeStars.pdf | PDF]] == OGLE and MACHO data were studied for Be stars.== * OGLE (LMC,SMC): [http://ukads.nottingham.ac.uk/abs/2005MNRAS.361.1055S Sabogal et al. 2005], [http://ukads.nottingham.ac.uk/abs/2006A%26A...457..949M Mennickent et al. 2006] * OGLE (Bulge): [http://ukads.nottingham.ac.uk/abs/2008A%26A...478..659S Sabogal et al. 2008] 29,000 found in OGLE-II Bulge fields. * MACHO: [http://ukads.nottingham.ac.uk/abs/2002AJ....124.2039K Keller et al. 2002] 1279 found in MACHO LMC data. [[File:Be-OGLE-CMD-Bulge.png|400px]] [[File:Be-OGLE-CMD-LMC.png|400px]] [[File:Be-OGLE-ampl.png|400px]] [[File:Be-OGLE-distributions.png|400px]] [[File:Be-OGLE-Type1.png|400px]] [[File:Be-OGLE-Type1-slow.png|400px]] [[File:Be-OGLE-Type2.png|400px]] [[File:Be-OGLE-Type1-2.png|400px]] [[File:Be-OGLE-Type3.png|400px]] [[File:Be-MACHO-modes.png|400px]] [[File:Be-MACHO-mixed-modes.png|400px]] [[File:Be-MACHO-spectra.png|600px]] aa6171f4e8a2b425c5c594a1de1fc4aa3b5ade74 6 180 1133 1047 2012-06-22T16:22:10Z Lukasz 2 uploaded a new version of &quot;[[File:SciAlertsBeStars.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 191 1138 1097 2012-07-16T09:40:49Z Lukasz 2 uploaded a new version of &quot;[[File:Poster2012.jpg]]&quot;: ESF logo added. wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1139 1138 2012-07-16T09:42:45Z Lukasz 2 uploaded a new version of &quot;[[File:Poster2012.jpg]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 182 1140 1071 2012-07-16T09:44:44Z Lukasz 2 /* Lunches and social dinner */ wikitext text/x-wiki =Travel info= == By Air == Bologna airport: [http://www.bologna-airport.it/uk/?LN=UK] Direct flights from major European cities, including London (Stansted, Heathrow, Gatwick), Paris, Brussels, Viena, Berlin, Frankfurt (main hub for trans-atlantic flights), Munich, Budapest, Poznan, Lisbon, Barcelona, Madrid, Istanbul. Within Italy direct flights from Rome Fiumicino, Naples, Palermo, Catania. == By Train == Trenitalia [http://www.trenitalia.com] operates very frequent trains from major Italian cities. From Roma Termini to Bologna Centrale: 2h, price from 19 euros. From Milano Centrale to Bologna Centrale: 2h, price from 19 euros From Venezia S.Lucia to Bologna Centrale: 1.5h, price from 19 euros; slow train: 2h, price from 10 euros From Firenze S.M.Novella or Campo Di Marte to Bologna Centrale: 0.5h, price from 19 euros =Workshop venue= Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33 (shown by an arrow on the map) Map of the University area: [[Media:BOmap.pdf|also in PDF]] [[File:BolognaMap.png| 500px]] Useful information and an interactive map to find how to get around Bologna can be found here: [http://www.atc.bo.it/english] =Accommodation= List of suggested accommodations (with breakfast included): '''Important: specify that you will participate to the meeting organised by "Osservatorio Astronomico di Bologna" to have the special rate indicated here.''' * Hotel Holiday (3 stars hotel) [http://www.hotelholiday-bo.com] Via Bertiera ,13. tel. 051235326 fax 051235326 Single room 55€ Double room 65 € * Hotel University (3 stars hotel) [http://www.hoteluniversitybologna.it] Via Mentana 7. tel. 051229713 fax 051229713 Single room 60€ Double room 76€ * Hotel San Donato (3 stars hotel) [http://www.hotelsandonato.it] e mail: info@hotelsandonato.it (fot the attention of Sig. Ricciotti) Via Zamboni,16. tel. 051235395 fax230547 Single room 70€ Double room 90€ * Hotel Paradise ( 3 stars hotel) [http://www.hotelparadisebologna.com] Via Cattani 7. tel. 051231792 fax 051234591 Single room 50€ Double room 70€ ''(prices valid for December 2011)'' <big>List of other hotels and restaurants [[Media:logisticsBologna2012.pdf | here]]</big> =Lunches and social dinner= The launches will be provided, possibly within the workshop's venue. Other suggested restaurants for lunch are: * 28- ALCE NERO -- Via Petroni 9/b – Tel: 2759196 * 19- CAFFE' UNIVERSITA' -- Via Zamboni 92 – Tel: 244 368 (lunch only) '''We plan the social dinner on Thursday evening at:''' * 6 - OSTERIA LA MATTA -- Via Zucchini 9/c -- Tel: 240177 2118ab5c28a6173ef2e5fdf36c4be54a2e4e58d2 0 195 1144 2012-07-16T09:47:29Z Lukasz 2 Created page with "Small version in JPG: [[Media:Poster2012.jpg]]" wikitext text/x-wiki Small version in JPG: [[Media:Poster2012.jpg]] f8cafef55a4316b3b1e1b4ed390e252cbec5d71b 1145 1144 2012-07-16T09:47:53Z Lukasz 2 wikitext text/x-wiki Small version in [[Media:Poster2012.jpg|JPG]] 73589e04ef8073ac85883817274b9c1adf0fa295 1146 1145 2012-07-16T09:48:40Z Lukasz 2 wikitext text/x-wiki [[File:Poster2012.jpg|300px]] * Small version in [[Media:Poster2012.jpg|JPG]] * Large version in [[Media:Poster2012big.png|PNG]] e9ffb65b1d76b29ee8cce9dc57caa555694ce15a 1148 1146 2012-07-16T09:49:43Z Lukasz 2 wikitext text/x-wiki [[File:Poster2012.jpg|300px]] * Small version in [[Media:Poster2012.jpg|JPG]] * Large version in [[Media:Poster2012big.png|PNG]] * Large version in [[Media:Poster2012big.tiff|TIFF]] The poster was designed and produced by Amanda Smith. 92559df68d003cae9d7a266a97e166a087d6b432 1149 1148 2012-07-16T09:51:07Z Lukasz 2 wikitext text/x-wiki [[File:Poster2012.jpg|300px]] * Small version in [[Media:Poster2012.jpg|JPG]] * Large version in [[Media:Poster2012big.png|PNG]] * Large version in [[Media:Poster2012big.pdf|PDF]] The poster was designed and produced by Amanda Smith. 3da1cee023fac18ce62b6feda32229a836041c75 6 196 1147 2012-07-16T09:49:07Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 197 1150 2012-07-16T09:51:39Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 188 1152 1151 2012-07-25T21:04:06Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa 5830d3f824fea3d2738e7899749b29e82b526974 1153 1152 2012-07-26T12:00:45Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb 27df72c84b99210ab489028b8fa3a3d3670b87a4 1158 1153 2012-07-30T04:56:48Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot 3a2de3f9b035f52af508ab13a7b945126fe520be 1160 1158 2012-08-03T20:44:54Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger 2f2fe2ef49025899beedb9419e9df9ad5f96be08 1161 1160 2012-08-06T20:41:03Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini b93063c4fc68ad81110a5c94ed2402e221ca2c1f 1162 1161 2012-08-07T12:34:35Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli e942c442aef331bbc0b32d3110ae9f1a27cdae15 1163 1162 2012-08-08T20:51:03Z Lukasz 2 /* Registration */ wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto 267b9ad038d9aa28b5f5b5ad95e6240b5aeb0ce5 1164 1163 2012-08-10T08:45:22Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi 437cf6f982411d6ed4e5d3c5d84786d0aff5f3c4 1165 1164 2012-08-10T19:22:50Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee brakes will be provided free of charge.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella 7b05d636917dc0217b205022583732481888f699 1166 1165 2012-08-13T15:17:50Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker dde44d3c5e4a8b1854ed16b9844f977cf02d08c4 1167 1166 2012-08-15T19:48:55Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration will close on the 15th of August 2012.'' ---- <big>[[Workshop2012:registrationform | Registration form]]</big> ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) 88e3e4e61a84ac903451449887c81afd5f0eab70 1168 1167 2012-08-17T19:57:43Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) b53ef9901397e7f6078a929feab1d3aefb0c8f46 1169 1168 2012-08-17T19:58:29Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov 01361d1d6b1fd5479561f4cc0a94fcd953e273a7 1170 1169 2012-08-20T12:29:39Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) 99d21513d0dd60fd05b148d443c485e7185b6d76 1171 1170 2012-08-20T15:36:56Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) # Elena Pacino 18bdda79eecd598b170a5dd99de9fcc36a4d7f3f 1176 1171 2012-08-21T12:53:28Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Cristina Valeria Torres # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi 51a971f1048ba965ac5355ac8b0404e3fbb9d845 1177 1176 2012-08-22T08:05:14Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Lina Tomasella # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi d6830a4581e7ff71acce406c901190395504ffec 1178 1177 2012-08-24T14:19:34Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi # Giuseppa Altavilla # Stefano Benetti 11df8b3dd4dbae4f03f2c53a86239dc0df62f48f 1191 1178 2012-08-27T18:00:18Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Iain Steele # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi # Giuseppa Altavilla # Stefano Benetti # Andreja Gomboc da2d028f7ad0ac52d1d9f3a9abbdf4233a987f24 1195 1191 2012-08-28T19:12:15Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Vasily Belokurov # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi # Giuseppa Altavilla # Stefano Benetti # Andreja Gomboc e747677d4284bc59845ea389ea1ad6fcf326c203 1196 1195 2012-08-28T19:12:39Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Eran Ofek # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi # Giuseppa Altavilla # Stefano Benetti # Andreja Gomboc 066cec7a64b818452dd11e168af41b86f746c9a5 0 17 1154 1131 2012-07-30T04:37:21Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[File:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 2445a84b3319906eb7fb5f8bcc7136d44718ea84 1156 1154 2012-07-30T04:43:47Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * availability of flux measurements within less than couple of hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 7e2f990582fc99ef4af20e38b8407256f4ca11c9 1157 1156 2012-07-30T04:46:13Z Lukasz 2 /* Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows for rough uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * da09fe83f90f0c8bce1dec8971001b3ce8d7c53c 6 194 1155 1127 2012-07-30T04:43:34Z Lukasz 2 uploaded a new version of &quot;[[File:GaiaFollowupServerManual.pdf]]&quot;: version of 30.July 2012. Updated http address of the server. wikitext text/x-wiki version of June 2012. a88ad5fcc354459febd089042467faaff874658b 0 189 1159 1077 2012-07-30T04:59:02Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gsaw2012@gmail.com'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 6th''''' ''in the Osteria la Matta'' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 6bae514f2b1114535956a7a37ade1451023e45d7 0 190 1172 1121 2012-08-21T12:33:08Z Lukasz 2 wikitext text/x-wiki '''Wednesday, September 5th''' Informal meetings at the Observatory from 9:30am - drafting the Memoranda of Understanding, individual discussions with potential partners. '''Thursday, September 6th''' First day of the meeting from 9:30am at the Observatory. Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Discussing the details of the operation during the verification phase, including Memorandums of Understanding * Presentation of tools for coordinated follow-up observations of transients The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 509920480ce5af8673f36b8c72a6a411426d9484 1173 1172 2012-08-21T12:34:54Z Lukasz 2 wikitext text/x-wiki '''Wednesday, September 5th''' '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Discussing the details of the operation during the verification phase, including Memorandums of Understanding * Presentation of tools for coordinated follow-up observations of transients The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 09e1c26421ebd5bc705daf253565f8dd9f486c26 1174 1173 2012-08-21T12:35:06Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day ---- ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Discussing the details of the operation during the verification phase, including Memorandums of Understanding * Presentation of tools for coordinated follow-up observations of transients The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 2d812f6688cf7d14f792e1c831b00a858925424f 1175 1174 2012-08-21T12:35:24Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- ---- Talks will cover the following-topics: * On-going large-scale surveys for transients (CRTS, PTF, PanStarrs, Skymapper, Super-WASP, ASAS, LOFAR, OGLE and others) * Future large-scale surveys for transients (Gaia, LSST) * Classification methods for transients * Reports from the follow-up observations of transients, sharing the experience * Presentations of Gaia Follow-Up Network partners * Discussing the details of the operation during the verification phase, including Memorandums of Understanding * Presentation of tools for coordinated follow-up observations of transients The list above is far from complete and the final agenda will be composed of contributions suggested by workshop's participants. 1ab8c4aa0d7888b60d550057c9913cdee859a376 1179 1175 2012-08-25T19:54:10Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- Draft agenda is available [[Media:Agenda-draft.pdf here]]. Please send comments/corrections to '''gsaw2012@gmail.com''' 3d2e53b1d767b15e39d12272f8c5f81280d2c2b0 1180 1179 2012-08-25T19:54:33Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- Draft agenda is available [[Media:Agenda-draft.pdf|here]]. Please send comments/corrections to '''gsaw2012@gmail.com''' 58726e7b0ff5a3d7145e2d4cb0340e70d212cd85 1181 1180 2012-08-25T19:55:04Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to '''gsaw2012@gmail.com''' 9b5bb939a51eaf49f048cadb9edb30965ff2d003 1183 1181 2012-08-25T19:55:31Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' bbedfa951ba2e4079c6c88254c84ba8eff30e4ea 1184 1183 2012-08-27T07:50:28Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- Draft agenda is available [[File:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' a484db7b975c32fd69ffb649531f908649942f23 1186 1184 2012-08-27T07:50:50Z Lukasz 2 wikitext text/x-wiki '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' bbedfa951ba2e4079c6c88254c84ba8eff30e4ea 1187 1186 2012-08-27T07:51:08Z Lukasz 2 wikitext text/x-wiki Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- 0d73c1d65fedec8626d109d0a35e94f5717678a1 1188 1187 2012-08-27T08:03:32Z Lukasz 2 wikitext text/x-wiki ---- Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- c60365f5cd9dac471a447cc06d244f89fd889e66 1190 1188 2012-08-27T08:15:48Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- e7baa7a752f172c8cb191fa347609542fbf4ed91 1192 1190 2012-08-28T10:14:11Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[File:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- 9241326efbfa850f7b201cf50468489643368457 1194 1192 2012-08-28T10:14:52Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- e7baa7a752f172c8cb191fa347609542fbf4ed91 1197 1194 2012-08-29T09:26:50Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[File:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- 603c8eca05651ff8a73b67a4ee45c19db9f892fe 1199 1197 2012-08-29T09:27:10Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- e7baa7a752f172c8cb191fa347609542fbf4ed91 1200 1199 2012-08-29T09:27:28Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- aa0d195c816ae301b2b3183e8a5977d3e858dbc8 1201 1200 2012-08-30T13:13:52Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[File:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- fc6e952b092fccf8668d27e9818fb6ea6929325a 6 198 1182 2012-08-25T19:55:14Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1185 1182 2012-08-27T07:50:40Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1193 1185 2012-08-28T10:14:27Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 199 1189 2012-08-27T08:03:43Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1198 1189 2012-08-29T09:27:02Z Lukasz 2 uploaded a new version of &quot;[[File:AbstractBook2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 198 1202 1193 2012-08-30T13:14:10Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1225 1202 2012-08-31T13:34:47Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1232 1225 2012-09-03T14:02:47Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1239 1232 2012-09-04T09:28:21Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1244 1239 2012-09-05T15:29:32Z Lukasz 2 uploaded a new version of &quot;[[File:Agenda2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 190 1203 1201 2012-08-30T13:14:27Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- aa0d195c816ae301b2b3183e8a5977d3e858dbc8 1224 1203 2012-08-31T13:34:35Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[File:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- fc6e952b092fccf8668d27e9818fb6ea6929325a 1226 1224 2012-08-31T13:35:03Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- 1cae7fb44e808b7c10c25a87cf2f6189c8762d37 1227 1226 2012-08-31T13:35:10Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- '''Thursday, September 6th''' First day of the meeting from 9:30am at the Aula della Specola, Università degli Studi di Bologna 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- aa0d195c816ae301b2b3183e8a5977d3e858dbc8 1228 1227 2012-09-01T19:43:39Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |RTS2: advances in last two years |Petr Kubanek |20m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:30 |The 1.8m telescope at Cima Ekar |Massimo Turatto |15m |---- |14:45 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:00 |The PIRATE facility |Ulrich Kolb |15m |---- |15:15 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:30 |'''''Coffee''''' | |30m |---- |16:00 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} 19:00 Social dinner at Osteria la Matta - Via Zucchini 9/c '''Friday, September 7th''' Second day - finish at 5pm. ---- 2fc0b2b1fe785b6e7b0be04495f656b0ac0ef368 1229 1228 2012-09-01T19:43:55Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |RTS2: advances in last two years |Petr Kubanek |20m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:30 |The 1.8m telescope at Cima Ekar |Massimo Turatto |15m |---- |14:45 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:00 |The PIRATE facility |Ulrich Kolb |15m |---- |15:15 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:30 |'''''Coffee''''' | |30m |---- |16:00 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} f003771e40db1a3b4ae958458f9f8b0db0b662db 1230 1229 2012-09-03T14:01:20Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} 5be8b82ed4c8dad109d608b2262cfb5b70bdb90d 1231 1230 2012-09-03T14:02:32Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[File:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} 00da30b07414b2699802570218ff3fae7bede654 1233 1231 2012-09-03T14:02:58Z Lukasz 2 wikitext text/x-wiki ---- <big>Draft agenda is available [[Media:Agenda2012-draft.pdf|here]]. Please send comments/corrections to ''gsaw2012@gmail.com'' ---- Draft version of the Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} 5be8b82ed4c8dad109d608b2262cfb5b70bdb90d 1234 1233 2012-09-03T14:04:43Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. </big> ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 0986720e7342a8ba62d660ac35a9adda925c50c3 1235 1234 2012-09-03T14:04:51Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]]. ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 8e08102fe51bb9368edfda5185e8d8435b887a5b 1236 1235 2012-09-03T14:05:00Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 95ef826c7747a9315dd8fe9f451c6db09ebf4444 1237 1236 2012-09-04T09:26:22Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 307c71654d13b0e3a4730de3fb034bf9b9acdd04 1238 1237 2012-09-04T09:28:07Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[File:Agenda2012-draft.pdf|here]] as a pdf.'' eeb8bbd4ec455dc3092b36b88f6f7e78bd0d147f 1240 1238 2012-09-04T09:28:59Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |20m |---- |10:20 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |10:40 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |11:50 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:10 |The Palomar Transient Factory, description and results |Eran Ofek |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 307c71654d13b0e3a4730de3fb034bf9b9acdd04 1245 1240 2012-09-05T15:32:00Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |25m |---- |10:25 |Gaia scanning law |Berry Holl |15m |---- |10:40 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:50 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |12:10 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:15 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' d3a2a5cbe93d0da0b63d143dc563cf640fb1f48a 1246 1245 2012-09-05T21:13:06Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |Gaia status |Timo Prusti |25m |---- |10:00 |Gaia science alerts status and introduction to the verification phase |Simon Hodgkin |25m |---- |10:25 |Gaia scanning law |Berry Holl |15m |---- |10:40 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:50 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |12:10 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' a931f675aa58883c46194acecd0bdbe11f08e14a 0 17 1204 1157 2012-08-30T16:08:53Z Sergey.koposov 30 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Here is the documentation on the [ Calibration_Server|Cambridge Photometry Calibration Server] <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * d6d5eb6636097ecf59969562064cbdbabd4b6335 1205 1204 2012-08-30T16:09:38Z Sergey.koposov 30 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] <big>'''Please refer to the [[Media:GaiaFollowupServerManual.pdf | Manual]] for details. '''</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 6318488bca5fe93c38644952e87c570e86ec4641 1206 1205 2012-08-30T16:10:12Z Sergey.koposov 30 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] There is also a keynote presentation about it [[Media:GaiaFollowupServerManual.pdf | Manual]]. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * d01430d8d2437eff949462d975b4cdc60aed6b2f 1207 1206 2012-08-30T16:10:31Z Sergey.koposov 30 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> There is also a keynote presentation about it [[Media:GaiaFollowupServerManual.pdf | Manual]]. If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * ec00981355a8e19c758429cf0a6cd668171de3df 0 200 1208 2012-08-30T16:12:13Z Sergey.koposov 30 Created page with "The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ * In order to access the server you need a so called "hashtag" which is an autorization key. In order to ge..." wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have eca3fcd5649aecae91df4ab8775e1d972d5d1e06 1209 1208 2012-08-30T16:12:44Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have == Headline text == 058bc2d89150215c92487170b8871644e8ec2474 1210 1209 2012-08-30T16:15:41Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" 55b2ff77ccea7acc1c82bcfa635a84aa95d94ad6 1211 1210 2012-08-30T16:17:37Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ 8be21fd8606d6e24ca2050133eaa3274221dac46 1212 1211 2012-08-30T16:21:53Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ 272cbbbf7bba9bdc102c437bec1a0167fb1db63b 1213 1212 2012-08-30T16:25:06Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. You can also see the light curves for those alerts which have followup data through those forms: dbb97f78253a7292a3e5cee2d494da4f948fd3bd 1214 1213 2012-08-30T16:25:34Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and report to him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. You can also see the light curves for those alerts which have followup data through those forms: 55f08f32b531193cb55c17b2a50d6de1657414ba 1215 1214 2012-08-30T16:28:13Z Sergey.koposov 30 wikitext text/x-wiki The main address at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 6494a49e279df15d7e10f5a3c6e54b0844ba17eb 1216 1215 2012-08-30T16:29:25Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 d27838196cf42ebfd9dbdcb47d430fbb4836d358 1217 1216 2012-08-30T16:29:41Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 750a4d2e623a220952f8f406069e4a5d4fd6ac63 1218 1217 2012-08-30T16:31:33Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@test/110621_V4.cat;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 aea3180d0cfcf16dad36035bf431395beccb5e94 1219 1218 2012-08-30T16:36:46Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 99f69a75aa68c847bbe666c9151ffe440cd2c4a2 1220 1219 2012-08-30T16:37:46Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 973fe6a0753beeeb251911e56cc3b6d317425123 1221 1220 2012-08-30T16:41:02Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the repository https://bitbucket.org/sega_sai/gaia_followup f8f7d478c1451ea5565407e53fa89b90ccc9c752 1222 1221 2012-08-30T16:41:55Z Sergey.koposov 30 /* Source code */ wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Autorization == * In order to access the server you need a so called "hashtag" which is an autorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org ef12f108a4f33be65094bb2d65ee76672ab22177 1223 1222 2012-08-30T16:42:24Z Sergey.koposov 30 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org e3d9f2db81761194d1486ef2c017e59ac5a87afd 6 199 1241 1198 2012-09-04T09:34:54Z Lukasz 2 uploaded a new version of &quot;[[File:AbstractBook2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1242 1241 2012-09-04T09:36:40Z Lukasz 2 uploaded a new version of &quot;[[File:AbstractBook2012-draft.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 188 1243 1196 2012-09-05T13:28:34Z Lukasz 2 wikitext text/x-wiki ==== Registration ==== Workshop will be limited to 40 attendees. The allocation of the places will be subject to registration application. '''It is a pleasure to announce that we obtained some support for the workshop from GREAT grant of ESF. Therefore there will be no registration fee, the lunches and coffee breaks will be provided free of charge. We are also able to provide some limited support for participants. Please fill the registration form and contact us if you require any support.''' ''Registration closed on the 15th of August 2012.'' Please contact ''gsaw2012@gmail.com'' if you would like to amend your registration. ---- List of participants: # Massimo Turatto # Minia Manteiga Outeiro # Petr Kubanek # Gianluca M Guidi # Vladimir Lipunov # Michel Dennefeld # Gerry Gilmore # Zsolt Paragi # Timo Prusti # Mario C. Diaz # Paola Di Matteo # Laurent Eyer # Lovro Palaversa # Ulrich Kolb # William Thuillot # Werner Zeilinger # Antonio Pasqua # Gisella Clementini # Valentina Zitelli # Isabella Pagano # Giuseppe Leto # Stefan Keller # Yogesh Chandra Joshi # Peter Jonker # Berry Holl # Andrew Drake # Tim Staley # George Seabroke # Ashish Mahabal (via skype) # Lukasz Wyrzykowski # Simon Hodgkin # Joseph Richards (via skype) # Elena Pacino # Simone Leonini # Paolo Rosi # Giuseppa Altavilla # Stefano Benetti # Andreja Gomboc 090755795cd8afd6cb4d0d78bc157c65b5f9ae8b 0 1 1247 1092 2012-09-07T21:24:42Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big>[[Workshop2012:main| Gaia Science Alerts Workshop 2012]]</Big>''' 6-7 September 2012, Bologna, Italy </center> ---- <center> [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- d74321a0da6d3f9298e758df5d2212ff9bd0962b 0 186 1248 1143 2012-09-07T21:26:43Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|300px]] 695651dcad31ed6441e57d86660d1559a8a43237 1249 1248 2012-09-07T21:26:58Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|300pix]] 54f2a5fec1c69e74753d56bf9a5538b46a7fb40c 1250 1249 2012-09-07T21:27:06Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop will be held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg 300pix]] 3153e1b2cf674d7e900a6e2e5e68e5b45228e1a9 1251 1250 2012-09-07T21:27:54Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|left|300px]] 070f8e0581cb38fc10307bbc4437c95bc75d3997 0 186 1252 1251 2012-09-07T21:28:36Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|right|300px]] 02ccf14170bedac544296afe1c40680f3bd9bbe9 1253 1252 2012-09-07T21:28:52Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|right|300px Workshop photo]] f3f313c35acfda74d8176f68f98851212d6bc81e 1254 1253 2012-09-07T21:29:05Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|left|300px|Workshop photo]] f95b91affec70034af5eca25542097d38c4df897 1256 1254 2012-09-07T21:32:09Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|left|600px|Workshop photo]] ea8c3e1bb634dac6d7242bf7289e8be67627c989 1257 1256 2012-09-07T21:32:24Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop Photo === [[File:GSAW2012photo.jpg|left|800px|Workshop photo]] 2850b121a7c06b4e7ca8ed50300fe515c5d2f7b2 1258 1257 2012-09-07T21:32:44Z Lukasz 2 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato [[File:GSAW2012photo.jpg|right|800px|Workshop photo]] e131e2e74616c5148b8c7ed16dfa25aefd68747c 1259 1258 2012-09-07T21:33:24Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2012:registration|Registration]] * [[workshop2012:logistics|Logistic information]] * [[workshop2012:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Gisella Clementini * Simon Hodgkin * Massimo Turatto * Gerry Gilmore * Caroline Soubiran LOC: * Giuseppe Altavilla * Sandra Caddeo * Valentina Zitelli * Diego Zuccato === Workshop photo === [[File:GSAW2012photo.jpg|left|800px|Workshop photo]] b7d239d12018da7ee6b5fb6dcf7b4440de19b79a 6 201 1255 2012-09-07T21:31:43Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 1 1260 1247 2012-09-17T09:46:48Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big></Big>''' </center> ---- <center> [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 2ae74365e13b299c9b8f086d19ef8263d6e98af7 0 190 1261 1246 2012-09-17T13:57:08Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |Gaia Spectro Science Alerts: first implementation plans |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Spectroscopic science alerts : possible triggers in the RVS domain |Paola Di Matteo |20m |---- |11:50 |Gaia-FUN-SSO: a network for Solar System transient objects |William Thuillot |20m |---- |12:10 |Open Transient Science and Future Prospects with CRTS |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |Global MASTER-Net |Vladimir Lipunov |20m |---- |14:50 |4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes |Tim Staley |20m |---- |15:10 |Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients |Peter Jonker |20m |---- |15:30 |Locating Transients with the e-EVN |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |The TOROS project |Mario C. Diaz |20m |---- |16:40 |Gravitational Wave research and their connection with EM observations |Gianluca M. Guidi |30m |---- |17:10 |Discussions on multi-messanger synergies | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 02d6573d49845a60d8b5f9abaac446d08897a809 1262 1261 2012-09-17T14:07:26Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA-Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' b59d3aac2984a5165604f69fec651fa911425f90 1263 1262 2012-09-17T20:19:54Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA-Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' edd91c4c835f11ae6ff861c761a20ff4003af871 1264 1263 2012-09-17T20:20:52Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |Transient discovery and classification for PTF and variable star classification |Joseph Richards |25m |---- |09:55 |Using field information to separate SNe and non-SNe |Ashish Mahabal |30m |---- |10:25 |Classification of alerts within the Gaia pipeline |Lukasz Wyrzykowski |15m |---- |10:40 |Analysis of outlying observations from Gaia CU8 classification pipeline |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |Responding to the Event Deluge with VOEventNet |Roy Williams |25m |---- |11:55 |Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |The 1.8m telescope at Cima Ekar and SN classification programme at Asiago |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |RTS2: advances in last two years |Petr Kubanek |20m |---- |14:35 |Observational facilities at INAF OA-Catania |Giuseppe Leto |15m |---- |14:50 |The Observing Facilities of the Vienna Observatory |Werner Zellinger |15m |---- |15:05 |The PIRATE facility |Ulrich Kolb |15m |---- |15:20 |Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussions on verification details | |1h |---- |17:00 |''end of day 2'' | | |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 2f3ebfbd66f1100f0e8a1e1f1bc929ab073b5a5c 1265 1264 2012-09-17T20:34:01Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} Additional slides: {| class="wikitable" |'''title''' |'''name''' |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf] Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' d7c5e5830e0bbead60501ec68368e34b3d55c785 1266 1265 2012-09-17T20:34:21Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} Additional slides: {| class="wikitable" |'''title''' |'''name''' |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf] Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 44c19bf690ee5b40a7f390b9dfb97ddc2c3bcdd3 1267 1266 2012-09-17T20:34:48Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} Additional slides: {| class="wikitable" |'''title''' |'''name''' |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 0bc4bbd8bf34cded269c154f794a93b919767484 1268 1267 2012-09-17T20:35:27Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 715cef2084b5b527c0681fcb33a7abbee79cc2c6 1269 1268 2012-09-17T20:37:00Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now provided below. After the workshop each title will be linking to pdf and video recording of the talk. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- Meeting will take place at the Aula della Specola, Università degli Studi di Bologna, Via Zamboni 33. ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- <big>Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 14543ddabc7f6ad6091aa5c8a7370a70e4339bf5 1270 1269 2012-09-17T20:45:28Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' e09d5c85c413a95b69a53f42c5dff5f39a4676fc 1274 1270 2012-09-24T10:23:15Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' d509c6ec50130db6ce3954a6183ca36789aaa065 1275 1274 2012-09-24T10:23:29Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' bdd5dc661c0d337a49d54b88f0b049b280505473 1276 1275 2012-09-24T10:23:45Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' d0f50b435096ebc0b39b811cf0faa8e8812948a2 1277 1276 2012-09-24T10:23:56Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 5e8083a0867c33995bbc9ec1d82acdfbf7c95346 1278 1277 2012-09-24T10:27:01Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/simonhodgkin-sciencealerts.mov rec] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/berryholl-scanning.mov rec] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/georgeseabroke-spectral-alerts.mov rec] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/paoladimateo-spectral-alerts.mov rec] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/williamthuillot-asteroidalerts.mov rec] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/adrewdrake-catalinasurvey.mov rec] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' c6269a3ee10f6837d81746e642a178f092ce6a9d 1279 1278 2012-09-24T10:28:15Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/simonhodgkin-sciencealerts.mov rec] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/berryholl-scanning.mov rec] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/georgeseabroke-spectral-alerts.mov rec] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/paoladimateo-spectral-alerts.mov rec] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/williamthuillot-asteroidalerts.mov rec] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/andrewdrake-catalinasurvey.mov rec] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' e6c4c59728ce4d228abe6606eb4baa576ca6c871 1280 1279 2012-09-24T10:35:15Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/simonhodgkin-sciencealerts.mov rec] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/berryholl-scanning.mov rec] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/georgeseabroke-spectral-alerts.mov rec] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/paoladimateo-spectral-alerts.mov rec] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/williamthuillot-asteroidalerts.mov rec] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/andrewdrake-catalinasurvey.mov rec] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/wladimirlipunov-masternet.mov rec] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timstaley-4pi-radio.mov rec] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/peterjonker-multi-messanger.mov rec] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/zsoltparagi-eEVNTransients.mov rec] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/mariodiaz-toros-gw.mov rec] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/gianlucaguidi-gw-ligo.mov rec] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/joeyrichards-classification-ptf.mov rec] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/ashishmahabal-classification-catalina.mov rec] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] (sorry, no recording) |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] (sorry, no recording) |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/roywilliams-voeventnet.mov rec] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/lukaszwyrzykowski-giusepealtavilla-calibrations-follow-up.mov rec] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/massimoturatto-asiagnosne.mov rec] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/elenapancino-nanosatellite.mov rec] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/petrkubanek-rts2.mov rec] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/giuseppeleto-catania.mov rec] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/wernerzeilinger-vienna.mov rec] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/ulrichkolb-pirate.mov rec] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/yogeshjoshi-nainital.mov rec] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/discussion-verification-hodgkin.mov rec] | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' c3b3c6f8699d05fa4dd2068fbcbf5b61e53ffe9e 1281 1280 2012-09-24T10:35:54Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/simonhodgkin-sciencealerts.mov rec] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/berryholl-scanning.mov rec] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/georgeseabroke-spectral-alerts.mov rec] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/paoladimateo-spectral-alerts.mov rec] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/williamthuillot-asteroidalerts.mov rec] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/andrewdrake-catalinasurvey.mov rec] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/wladimirlipunov-masternet.mov rec] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timstaley-4pi-radio.mov rec] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/peterjonker-multi-messanger.mov rec] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/zsoltparagi-eEVNTransients.mov rec] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/mariodiaz-toros-gw.mov rec] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/gianlucaguidi-gw-ligo.mov rec] |Gianluca M. Guidi |30m |---- |17:10 |Discussion | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/joeyrichards-classification-ptf.mov rec] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/ashishmahabal-classification-catalina.mov rec] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] (sorry, no recording) |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] (sorry, no recording) |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/roywilliams-voeventnet.mov rec] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/lukaszwyrzykowski-giusepealtavilla-calibrations-follow-up.mov rec] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/massimoturatto-asiagnosne.mov rec] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/elenapancino-nanosatellite.mov rec] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/petrkubanek-rts2.mov rec] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/giuseppeleto-catania.mov rec] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/wernerzeilinger-vienna.mov rec] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/urlichkolb-pirate.mov rec] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/yogeshjoshi-nainital.mov rec] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/discussion-verification-hodgkin.mov rec] | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 02e8ad316c95c48df747b878c0080d2963f49855 1282 1281 2012-09-24T10:37:41Z Lukasz 2 wikitext text/x-wiki The agenda of the workshop is now acting as an archive of the presentations. Each title is linked to a pdf version. Where available, the video or audio recording is linked after the title. ---- '''Abstract Book is available [[Media:AbstractBook2012-draft.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Thursday, September 6th''' |---- |09:30 |Welcome |LW+STH+GC+MT |5m |---- |09:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Prusti-Alerts.pdf Gaia status] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timoprusti-gaia.mov rec] |Timo Prusti |25m |---- |10:00 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/hodgkinbologna2012.pdf Gaia science alerts status and introduction to the verification phase] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/simonhodgkin-sciencealerts.mov rec] |Simon Hodgkin |25m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/BH_ScienceAlertsScanningLaw.pdf Gaia scanning law] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/berryholl-scanning.mov rec] |Berry Holl |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/seabroke_alerts_bologna.pdf Gaia Spectro Science Alerts: first implementation plans] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/georgeseabroke-spectral-alerts.mov rec] |George Seabroke |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/alerts_CU6_dimatteo.pdf Spectroscopic science alerts : possible triggers in the RVS domain] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/paoladimateo-spectral-alerts.mov rec] |Paola Di Matteo |20m |---- |11:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamThuillot-Gaia-Sc-Alerts-2012.pdf Gaia-FUN-SSO: a network for Solar System transient objects] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/williamthuillot-asteroidalerts.mov rec] |William Thuillot |20m |---- |12:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/drake_CRTS_Gaia.pdf Open Transient Science and Future Prospects with CRTS] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/andrewdrake-catalinasurvey.mov rec] |Andrew Drake |20m |---- |12:30 |'''''Lunch''''' | |2h |---- |14:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Lipunov-Bologna2012.pdf Global MASTER-Net] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/wladimirlipunov-masternet.mov rec] |Vladimir Lipunov |20m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Staley_4_pi_sky.pdf 4 Pi Sky of radio coverage: Transient discovery and response with next generation radio telescopes] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/timstaley-4pi-radio.mov rec] |Tim Staley |20m |---- |15:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GAIA-LOFAR-TKP-Sept2012.pdf Multi-messenger and multi-wavelength follow-up of LOFAR discovered transients] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/peterjonker-multi-messanger.mov rec] |Peter Jonker |20m |---- |15:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/e-EVN_GAIA_Science_Alerts.pdf Locating Transients with the e-EVN] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/zsoltparagi-eEVNTransients.mov rec] |Zsolt Paragi |20m |---- |15:50 |'''''Coffee''''' | |30m |---- |16:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Diaz-TOROS-GAIA-workshop.pdf The TOROS project] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/mariodiaz-toros-gw.mov rec] |Mario C. Diaz |20m |---- |16:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Guidi-GaiaScienceAlertsWorkshop-Bologna.pdf Gravitational Wave research and their connection with EM observations] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/gianlucaguidi-gw-ligo.mov rec] |Gianluca M. Guidi |30m |---- |17:10 |Discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/discussion-verification-hodgkin.mov rec] | | |---- |18:00 |''end of day 1'' | | |---- |19:00 |colspan="3"|'''''Dinner at Osteria la Matta - Via Zucchini 9/c''''' |---- | |---- |colspan="4"|'''Friday, September 7th''' |---- |09:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/joeyrichards_ptf_classify.pdf Transient discovery and classification for PTF and variable star classification] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/joeyrichards-classification-ptf.mov rec] |Joseph Richards |25m |---- |09:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Mahabal_20120907_Gaia2012.pdf Using field information to separate SNe and non-SNe] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/ashishmahabal-classification-catalina.mov rec] |Ashish Mahabal |30m |---- |10:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-ClassificationinGaia.pdf Classification of alerts within the Gaia pipeline] (sorry, no recording) |Lukasz Wyrzykowski |15m |---- |10:40 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GSA2012-CU8-Outliers-Manteiga.pdf Analysis of outlying observations from Gaia CU8 classification pipeline] (sorry, no recording) |Minia Manteiga Outeiro |20m |---- |11:00 |'''''Coffee''''' | |30m |---- |11:30 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/WilliamsGaiaBologna.pdf Responding to the Event Deluge with VOEventNet] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/roywilliams-voeventnet.mov rec] |Roy Williams |25m |---- |11:55 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/LW-Bologna-Verification.pdf Cambridge Photometric Follow-up Calibration Server- report from tests and verification phase arrangements] [http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Altavilla_GaiaAlerts2012.pdf Report of Giuseppe Altavilla] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/lukaszwyrzykowski-giusepealtavilla-calibrations-follow-up.mov rec] |Lukasz Wyrzykowski/Giuseppe Altavilla |30m |---- |12:25 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/MTuratto_2012_Gaia_Bologna_2.pdf The 1.8m telescope at Cima Ekar and SN classification programme at Asiago] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/massimoturatto-asiagosne.mov rec] |Massimo Turatto |20m |---- |12:45 |'''''Lunch''''' | |1h 30m |---- |14:10 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/nanosat@GSA2012.pdf NanoSat] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/elenapancino-nanosatellite.mov rec] |Elena Pancino |5m |---- |14:15 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/rts2-advances.pdf RTS2: advances in last two years] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/petrkubanek-rts2.mov rec] |Petr Kubanek |20m |---- |14:35 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Letogaia-bo-sept62012.pdf Observational facilities at INAF OA-Catania] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/giuseppeleto-catania.mov rec] |Giuseppe Leto |15m |---- |14:50 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Zeilinger-WiennaTel.pdf The Observing Facilities of the Vienna Observatory] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/wernerzeilinger-vienna.mov rec] |Werner Zellinger |15m |---- |15:05 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/PIRATE-Bologna_Sept2012.pdf The PIRATE facility] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/urlichkolb-pirate.mov rec] |Ulrich Kolb |15m |---- |15:20 |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/yogesh-talk_gaia_ycj.pdf Synergy of GAIA mission with the Devasthal Optical Telescopes for follow-up observations] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/yogeshjoshi-nainital.mov rec] |Yogesh Chandra Joshi |15m |---- |15:35 |'''''Coffee''''' | |30m |---- |16:05 |Discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2012/videos/discussion2.mov rec] | |1h |---- |17:00 |''end of day 2'' | | |} {| class="wikitable" |---- |colspan="2"|'''Additional related slides''' |---- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/Ashish-Calibrations.pdf Report on photometric follow-up calibrations] |Ashish Mahabal (Caltech) |--- |[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/GSAW2012/Talks/GROND_Greiner_4Gaia.pdf GROND. Capabilities for transients follow-up] |Jochen Greiner (MPE) |} ---- Agenda is available [[Media:Agenda2012-draft.pdf|here]] as a pdf.'' 7cee3c06ded7d2768fc30afdc6670cf9f84af5f9 0 17 1271 1207 2012-09-19T07:46:08Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] Here is the presentation about it [[Media:GaiaFollowupServerManual.pdf | Manual]].</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 999d4fa793def1b799abc08047a1511ca7e4d427 1272 1271 2012-09-19T07:46:24Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big>Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]].</big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * eec10f126555eb046fa62564f386f453aeddddda 1273 1272 2012-09-19T07:47:04Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h == Current and future instruments suitable for Gaia alerts response == '''Please expand this list with information on the telescopes/surveys which might be suitable and interested in Gaia alerts follow-up and in operation in years 2012-2017.''' [http://www.uni-sw.gwdg.de/~hessman/MONET/links.html Hessman's list] of (mainly robotic) telescopes (including ones in preparation). * MASTER Robotic Net ([http://arxiv.org/abs/0907.0827 Lipunov et al. 2009]) limiting mag= 19-20, started in 2002 in Moscow, Russia, followed-up many GCN alerts; now being upgraded to a network all over Russia (1000 clear nights per year). * 3 telescopes operated at the Konkoly Observatory, Piszkesteto Mountain Station [http://www.konkoly.hu/staff/racz/piszkesteto.html] (Hungary): 50 cm Cassegrain, 60/90/180 cm Schmidt, 1m RCC. * [http://www.bo.astro.it/loiano/index.htm Loiano] [http://www.bo.astro.it/loiano/152cm.html 1.52m Cassini Telescope] + [http://www.bo.astro.it/~loiano/TechPage/pagine/BfoscManualTechPage/BfoscManual.htm BFOSC] - Photometry + Spectroscopy, Lat. 44 15 33 N, Long. 11 20 02 E, 785m asl - [http://www.oabo.inaf.it/ INAF - Astronomical Observatory of Bologna] * 1b9505088b3ba0f408e91b72bf75fbfa7484947c 0 11 1283 1108 2012-10-03T20:12:51Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[Media:ScienceAlerts-timeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] f504ba7bb9de799de3fbea406c4779b78e6f79ae 1284 1283 2012-10-03T20:12:59Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[Media:ScienceAlerts-timeline.png|700px]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 84722c2588d254686a934ba38d94886b6a2187d4 1286 1284 2012-10-08T20:48:04Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[Media:ScienceAlerts-timeline.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 0094a33a83bb8a25481d31112adff28980dc301d 1287 1286 2012-10-08T20:48:18Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 9d64837af3b4cb75bdeec71dbcca8406028d6313 1288 1287 2012-10-08T20:48:33Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[Media:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] f2d194637a6b14a176cac9b7cb242510a894bfe2 1289 1288 2012-10-08T20:48:49Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[Media:ScienceAlerts-timeline.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 0094a33a83bb8a25481d31112adff28980dc301d 1290 1289 2012-10-08T20:49:05Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 2256ab70621e95475ad605c6b8f845333e6296d9 1293 1290 2012-10-08T20:51:28Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 9d64837af3b4cb75bdeec71dbcca8406028d6313 1294 1293 2012-10-08T20:52:32Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[Media:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] f2d194637a6b14a176cac9b7cb242510a894bfe2 1295 1294 2012-10-08T20:52:43Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 9d64837af3b4cb75bdeec71dbcca8406028d6313 1297 1295 2012-10-08T21:15:00Z Lukasz 2 wikitext text/x-wiki [[Media:verificationbrochure.pdf | Verification brochure]] The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] ac5812ffa1fd5714a116a45509eb0e5e4c1bb276 1298 1297 2012-10-08T21:15:30Z Lukasz 2 wikitext text/x-wiki <big>[[Media:verificationbrochure.pdf | Verification brochure]]</big> The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 3d55d739d13445bf464deb824fd6ed0a89e06616 6 202 1285 2012-10-03T20:13:28Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 181 1291 1124 2012-10-08T20:49:35Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1292 1291 2012-10-08T20:51:07Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1296 1292 2012-10-08T20:53:01Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 203 1299 2012-10-08T21:15:46Z Lukasz 2 Created page with " == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Lau..." wikitext text/x-wiki == Preliminary list of telescopes and people involved == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} fe93008e02560736d25a2ff4372640baaaa4e562 1300 1299 2012-10-08T21:16:19Z Lukasz 2 wikitext text/x-wiki == Status of the partners preparing for the Gaia Alerts verification == {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} 3cd027e6f79ac955d3bd5bacf50314a849c83622 1301 1300 2012-10-08T21:18:07Z Lukasz 2 wikitext text/x-wiki == Status of the partners preparing for the Gaia Alerts verification == === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} 9ab23fd49c7211a035e3e14488b61d0620e8b35a 0 203 1302 1301 2012-10-09T07:03:59Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} 9829c4f137ccbe82a3be914e9cc0ba4a0937e526 1303 1302 2012-10-09T07:04:19Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 tests before June 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} ace54e86ff4555b045e3c02870e4c2455e8f30af 1304 1303 2012-10-09T07:04:33Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before June 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m {| border="1" style="width:85%;" !Telescope/Observatory || Contact person (with email) || Details |- |Swiss Euler || Laurent Eyer (laurent.eyer unige.ch) || 1.2m, La Silla, Chile |- |Belgian Mecatore || Laurent Eyer || 1.2m, La Palma (Swiss Time) |- |Bologna || Gisella Clementini (gisella.clementini oabo.inaf.it) || 1.5m, Loiano, Italy |- |Padova || Gisella Clementini || 1.82m reflector, Asiago, Italy |- |Catania || Gisella Clementini || robotic 80cm Ritchey-Cretien (APT2), Serra la Nave, Catania, Sicily |- |TNT Teramo || Anna Piersimoni (piersimoni oa-teramo.inaf.it) || 72cm Ritchey-Cretien, Central Italy |- |Konkoly || Laszlo Szabados (szabados konkoly.hu) || 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain, Piszkesteto Mountain Station of the Konkoly Obs., Hungary |- |} 4235333a9899ec3f8e0230a2a5c0fc3aa5c00736 1305 1304 2012-10-09T07:08:21Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before June 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m '''TESTS:''' ** 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain e39efa5164f62cd8a612d7f111b58d533a7c3831 1306 1305 2012-10-09T07:08:42Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before June 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain 8ef87beabbbc43e50616c2dd66760688afc7d3aa 1310 1306 2012-10-19T08:29:11Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain caadd6720b0c69f2ff8d570a6f3e8e4981267193 1311 1310 2012-10-19T08:30:49Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ea8d65ffc3e3ce5ac4d1ae9a49f8943694641f91 1312 1311 2012-10-19T19:23:20Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ad4b6eef0186359a4b697fb6d32bf376cb44bae0 1313 1312 2012-10-25T12:39:28Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs === GROND === * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 09d553d0cd58062572fffa9b15891319105f9b01 1314 1313 2012-10-25T12:44:10Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. ''(*) Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs === GROND === * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK cb82acb6424b34ef250f06dee61b936529741002 1315 1314 2012-10-25T12:44:25Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs === GROND === * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK e35b2530b6de1f3ceee0786a8ccb7a269ccd61fc 1316 1315 2012-10-29T15:45:10Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Target: [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html CSS121011:163803+372814] Participants: PIRATE, Belgian, pt5m, Loiano, ?? == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs === GROND === * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 62c23632f4d08571980641f4709a9dcb3a1292c3 1317 1316 2012-10-29T15:45:30Z Lukasz 2 /* Test no 1 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Target: [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html CSS121011:163803+372814] Participants: PIRATE, Belgian, pt5m, Loiano, ?? == Partners in test== === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs === GROND === * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK daf233bccd5cccce7d393021314a3a02f4b84c07 1318 1317 2012-10-29T20:55:21Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Target: [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html CSS121011:163803+372814] Participants: PIRATE, Belgian, pt5m, Loiano, ?? == Partners in test== === '''NORTH''' === === Loiano === * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 === Asiago=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m === APT2=== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien === TNT === * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien === Belgian Mercatore === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ===Konkoly=== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain === '''SOUTH''' === === Swiss Euler === * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ===Danish/Czech Telescope === * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs === GROND === * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK eb72c6eae513f66835ac6e13168fe2d382d8893e 1319 1318 2012-10-29T20:56:06Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Target: [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html CSS121011:163803+372814] Participants: PIRATE, Belgian, pt5m, Loiano, ?? == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 1932fc127e50f805b80b6f952627445a395044d0 1320 1319 2012-10-30T21:47:18Z Lukasz 2 /* Test no 1 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Target: [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html CSS121011:163803+372814] Participants: PIRATE, Belgian, pt5m, Loiano, Asiago == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 8d77def4d43b7c28cc375dde301bc7930b2ffe81 1321 1320 2012-11-02T21:16:04Z Lukasz 2 /* Test no 1 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html CSS121011:163803+372814] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 05387fdead981f1b40f6cf516a9e8492fd3cf5cd 1322 1321 2012-11-02T21:16:22Z Lukasz 2 /* Test no 1 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 16cf87b632c0139a78aecbd37fdd0194d9b90c64 0 17 1307 1273 2012-10-16T00:01:01Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 2 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 12h aae89344bf478071839f2b0fa681ef22dfe22c64 0 11 1308 1298 2012-10-19T08:23:41Z Lukasz 2 wikitext text/x-wiki Concise pack of information is available in the <big>[[Media:verificationbrochure.pdf | Verification brochure]]</big> ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 799e219fa72295b82f7218f331b928bb55feed5d 1309 1308 2012-10-19T08:24:07Z Lukasz 2 wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] ba8379052dcb30d9126dda918e9cd9250af91d28 1325 1309 2013-02-04T12:47:13Z Lukasz 2 wikitext text/x-wiki '''<big>Concise pack of information is available in the [[File:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 850575cfc4915cd4e53f8d686fce5c37e5d7a721 1327 1325 2013-02-04T12:47:52Z Lukasz 2 wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] ba8379052dcb30d9126dda918e9cd9250af91d28 1328 1327 2013-02-06T12:29:43Z Lukasz 2 wikitext text/x-wiki '''<big>Concise pack of information is available in the [[File:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 850575cfc4915cd4e53f8d686fce5c37e5d7a721 1330 1328 2013-02-06T12:30:41Z Lukasz 2 wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] ba8379052dcb30d9126dda918e9cd9250af91d28 0 200 1323 1223 2013-02-01T12:26:10Z Nadia 27 wikitext text/x-wiki The main address of the server at the moment is: http://gaia020.ast.cam.ac.uk:5000/ == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * IMPORTANT! The following fields must be selected in sextractor ''default.param'' file: [MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000] * Upload the sextractor output catalogue (by default ''test.cat'') to the Cambridge Photomretric Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gaia020.ast.cam.ac.uk:5000/uploader/ You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gaia020.ast.cam.ac.uk:5000/cgi/upload" Parameters of the http://gaia020.ast.cam.ac.uk:5000/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gaia020.ast.cam.ac.uk:5000/list_of_alerts ). If the alert is not in our DB, you can insert it http://gaia020.ast.cam.ac.uk:5000/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_followups You can view the list of alerts which are in the DB http://gaia020.ast.cam.ac.uk:5000/list_of_alerts , and the subset of them which have followup data http://gaia020.ast.cam.ac.uk:5000/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gaia020.ast.cam.ac.uk:5000/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 0c81bf6c95025777029161f9e3dea2954e693fda 6 181 1324 1296 2013-02-04T12:46:22Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 202 1326 1285 2013-02-04T12:47:37Z Lukasz 2 uploaded a new version of &quot;[[File:Verificationbrochure.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1329 1326 2013-02-06T12:30:26Z Lukasz 2 uploaded a new version of &quot;[[File:Verificationbrochure.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 1 1331 1260 2013-04-11T14:26:58Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big>4th Gaia Science Alerts Workshop 2013</Big>''' IAP, Paris, 19-21 June 2013 </center> ---- <center> [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- c07d34e47fff497d95eb6f450c8998fec37b556d 1332 1331 2013-04-11T14:27:26Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big>[[Workshop2013:main|4th Gaia Science Alerts Workshop 2013]]</Big>''' '''IAP, Paris, 19-21 June 2013''' </center> ---- <center> [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- fcd575c9b02034be34583539e0fd59c9cf021142 0 204 1333 2013-04-11T14:29:00Z Lukasz 2 Created page with "== Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topi..." wikitext text/x-wiki == Welcome! == [[File:Poster2012.jpg|right|300px]] '''The third Gaia Science Alerts workshop was held in [[Workshop2012:logistics | Bologna on 6-7 September 2012]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2012:rationale|Rationale]] * [[workshop2012:agenda|Agenda]] * [[workshop2013:registration|Registration]] * [[workshop2013:logistics|Logistic information]] %* [[workshop2013:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore LOC: * TDB d9eda8e996a13b3ae7cfbabd1584bf56297c3ced 1334 1333 2013-04-11T14:30:55Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop will be held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics this year include: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda]] * [[workshop2013:registration|Registration]] * [[workshop2013:logistics|Logistic information]] %* [[workshop2013:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore LOC: * TDB 1ddffd663d6883673af51db14a46f1d46ae68e16 1335 1334 2013-04-11T14:31:40Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop will be held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics this year include: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda]] * [[workshop2013:registration|Registration]] * [[workshop2013:logistics|Logistic information]] <--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore LOC: * TDB bb86ebc42b28d88e0b56a8b5ffb45497f4877d25 1336 1335 2013-04-11T14:31:53Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop will be held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics this year include: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda]] * [[workshop2013:registration|Registration]] * [[workshop2013:logistics|Logistic information]] -->* [[workshop2013:poster|Workshop's poster for download]] <-- ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore LOC: * TDB ff917ca9b1065ecec3d611b4ef72c4a30608f107 1337 1336 2013-04-11T14:32:41Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop will be held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics this year include: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda]] * [[workshop2013:registration|Registration]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore LOC: * TDB d55ac4c00ef67fe3acc9187a4602919fad5bd4f2 8 3 1338 1052 2013-04-11T14:35:47Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *; workshop 2013 **; workshop2013:main|Main Workshop Page **; workshop2013:rationale|Rationale **; workshop2013:agenda|Agenda **; workshop2013:registration|Registration / Participants **; workshop2013:logistics|Logistics * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 1f596820ffa28b40d86be2dac2f5ffac7c509150 1339 1338 2013-04-11T14:35:58Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2013 **; workshop2013:main|Main Workshop Page **; workshop2013:rationale|Rationale **; workshop2013:agenda|Agenda **; workshop2013:registration|Registration / Participants **; workshop2013:logistics|Logistics * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX e98311e5c0905b00e4a6bb9def93e13968582f44 1340 1339 2013-04-11T14:36:12Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2013 ** workshop2013:main|Main Workshop Page ** workshop2013:rationale|Rationale ** workshop2013:agenda|Agenda ** workshop2013:registration|Registration / Participants ** workshop2013:logistics|Logistics ; workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 9939a6e8111f4d42f26f23b2d90ab716c610e451 1341 1340 2013-04-11T14:36:22Z Gsawgwikiadmin 1 wikitext text/x-wiki * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2013 ** workshop2013:main|Main Workshop Page ** workshop2013:rationale|Rationale ** workshop2013:agenda|Agenda ** workshop2013:registration|Registration / Participants ** workshop2013:logistics|Logistics * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 3714621aec4a68ea6b5a9305033f1d0269643297 1342 1341 2013-04-11T14:37:13Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2013 ** workshop2013:main|Main Workshop Page ** workshop2013:rationale|Rationale ** workshop2013:agenda|Agenda ** workshop2013:registration|Registration / Participants ** workshop2013:logistics|Logistics * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 40bda2c89be3ebf2b8e3d5843d5342b24b813dd0 0 205 1343 2013-04-19T10:22:44Z Gsawgwikiadmin 1 Reg form installed wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiasciencealertsworkshop2013@gmail.com'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 20th''''' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 31cb7800cbd70d93c30e392d82b3ca7f02113d7d 1344 1343 2013-04-19T14:25:14Z Lukasz 2 Replaced content with "[[Workshop2013:registrationform]]" wikitext text/x-wiki [[Workshop2013:registrationform]] d8e6840286ac0fe26b8b9436aafb65605810da5e 1346 1344 2013-04-19T14:26:49Z Lukasz 2 wikitext text/x-wiki [[Workshop2013:registrationform | Registration form]] '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands 1eb59bc98487bd7420259099d59e7229e1d569f4 1347 1346 2013-04-19T14:27:01Z Lukasz 2 wikitext text/x-wiki <big>[[Workshop2013:registrationform | Registration form]]</big> '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands 34ac9aac1fb74e64510ed1efb371a2eb65f57924 1348 1347 2013-04-19T14:27:13Z Lukasz 2 wikitext text/x-wiki Please register here: <big>[[Workshop2013:registrationform | Registration form]]</big> '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands 9019eb4addcdd07434b9583e6db97e2fe4276a63 1349 1348 2013-04-19T14:27:23Z Lukasz 2 wikitext text/x-wiki '''Please register here: <big>[[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands 3896ddc67a484be00ed9a812d9dbed8999ecf7a6 1350 1349 2013-04-19T14:27:34Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands f097a24b2fd1d16904a8e49261a959ea10c7f1cd 0 206 1345 2013-04-19T14:25:19Z Lukasz 2 Created page with "== Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiascienc..." wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiasciencealertsworkshop2013@gmail.com'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *poster *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 20th''''' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 31cb7800cbd70d93c30e392d82b3ca7f02113d7d 0 207 1351 2013-04-19T14:28:32Z Lukasz 2 Created page with "'''Workshop announcement:''' Gaia will be ESA's milestone astrometric mission, and is due for launch in Autumn 2013. The final results from this billion stars survey are expecte..." wikitext text/x-wiki '''Workshop announcement:''' Gaia will be ESA's milestone astrometric mission, and is due for launch in Autumn 2013. The final results from this billion stars survey are expected in around 2020. Gaia will repeatedly map the whole sky and will find many transient events, including supernovae, novae, microlensing events, quasar flares, etc. Getting ready for this influx of Gaia data is now very timely and essential. We would like to invite you to the 4th Gaia Science Alerts Workshop, which will take place at the IAP in Paris, on 19-21 June 2013. During the workshop we will present the current status of the Gaia mission with an emphasis on developments in the alert pipeline and the capabilities of Gaia as a transient survey. The main part of the workshop will be devoted to the organisation of a dedicated follow-up observing team, which will conduct the verification of the alerts, and produce the first scientific results, from Gaia in 2014. The workshop will be an opportunity for presenting the partners and learning how to get involved in the follow-up of Gaia alerts. This year's workshop is also the first meeting within the EC's OPTICON Time Domain Work Package. The overall plan of this WP is to encourage small and medium telescopes to take part in coordinated time-domain astronomical observations. The Gaia alerts verification team will be the first body to be supported by the OPTICON. Please note that a limited support for participation in the workshop will be available. There will be no registration fee. 8a5045204f800e4c5e9da8a813aed5d623d628d3 0 208 1352 2013-04-19T14:29:47Z Lukasz 2 Created page with "The topics this year include: *Status of Gaia - year of the launch! *Prospects for Gaia alerts *Preparation for the alerts follow-up and verification *Follow-up strategies *Curr..." wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Prospects for Gaia alerts *Preparation for the alerts follow-up and verification *Follow-up strategies *Current/planned multi-wavelength transient surveys *Reports from tests on transient follow-up *Presentation of new partners 9cf8464455ae6b7afdbcbcd7d500999f57f4e105 1358 1352 2013-05-06T11:31:01Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Prospects for Gaia alerts *Preparation for the alerts follow-up and verification *Follow-up strategies *Current/planned multi-wavelength transient surveys *Reports from tests on transient follow-up *Presentation of new partners Draft Agenda: Wed 19. June: * lunch * welcome and session I * coffee break * session II Thu 20.June: * session III * coffee break * session IV * lunch * session V * coffee break * session VI * social dinner Fri 21.June: * session VII * coffee break * session VIII * lunch and end of the workshop cbfbd0ec0aa31194e6da1ca8271655327a67e30a 1359 1358 2013-05-06T11:31:33Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Prospects for Gaia alerts *Preparation for the alerts follow-up and verification *Follow-up strategies *Current/planned multi-wavelength transient surveys *Reports from tests on transient follow-up *Presentation of new partners == Draft Agenda == Wed 19. June: * lunch * welcome and session I * coffee break * session II Thu 20.June: * session III * coffee break * session IV * lunch * session V * coffee break * session VI * social dinner Fri 21.June: * session VII * coffee break * session VIII * lunch and end of the workshop 3639cb36cb30ea3f2f53bf64194111dedbe17c71 1360 1359 2013-05-06T11:31:52Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Prospects for Gaia alerts *Preparation for the alerts follow-up and verification *Follow-up strategies *Current/planned multi-wavelength transient surveys *Reports from tests on transient follow-up *Presentation of new partners == Draft Agenda == '''Wed 19. June:''' * lunch * welcome and session I * coffee break * session II '''Thu 20.June:''' * session III * coffee break * session IV * lunch * session V * coffee break * session VI * social dinner '''Fri 21.June:''' * session VII * coffee break * session VIII * lunch and end of the workshop 689c7041eaaff2ff3f359c6585fd86bc169663ce 1389 1360 2013-05-22T14:51:05Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Prospects for Gaia alerts *Preparation for the alerts follow-up and verification *Follow-up strategies *Current/planned multi-wavelength transient surveys *Reports from tests on transient follow-up *Presentation of new partners == Draft Agenda == '''Wed 19. June:''' * lunch * welcome and session I * coffee break * session II '''Thu 20.June:''' * session III * coffee break * session IV * lunch (provided by the organizers) * session V * coffee break * session VI * social dinner '''Fri 21.June:''' * session VII * coffee break * session VIII * lunch and end of the workshop 560989242b265d2165bd55040d721ef69d658988 0 205 1353 1350 2013-04-24T19:24:33Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary 9270cf6ecb798b2e80009f305e573b9f4950838f 1354 1353 2013-04-26T12:35:44Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey 823527947c312b914e7c1401e436aa9f548934ea 1355 1354 2013-04-29T19:48:13Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA ab050b7d4b5e2b91e7208f2c84c748339e9f910e 1356 1355 2013-05-01T20:03:08Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO 4482979e22f930262f412372731cf85e55ee1f6e 1357 1356 2013-05-02T20:34:06Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO # Paolo Tanga, Observatoire de la Côte d'Azur, France fb1962acd54d29176f11cc42a2724f210b75728a 1380 1357 2013-05-07T10:51:00Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh 7741a289b9d971c11658dcc9494ccb3a67a9d0d7 1381 1380 2013-05-07T15:25:58Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK 39c4a5283b59f37c146e0a8ff539ccee1b85fa92 1382 1381 2013-05-07T19:13:39Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France eeb92390f677049b4b1ae4347365b2d28c43e5cc 1383 1382 2013-05-09T22:01:33Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK 45d456fbcf04753030c7a35a705ed628802267ce 1384 1383 2013-05-13T14:20:35Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory 47cc6027044d10662d3dd7d35e6ddbc1db182294 1385 1384 2013-05-16T15:37:48Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK 697f061cddf58738ddf36feb40d5a24565806502 1386 1385 2013-05-19T21:30:50Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel b064df975227b5dbdfd4cd9225582901d98eea68 1387 1386 2013-05-20T08:44:40Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK 63d05e93578b9833f8473b4bf7e6c38502821c3a 1388 1387 2013-05-20T10:05:05Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK 76c1eddbbd54e0804da960299604b0f90fbb689e 1390 1388 2013-05-23T12:16:17Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA 3c1293f9009275828f61d7de42a75640e61d0d36 1391 1390 2013-05-23T14:19:14Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France b33e718123e02878a3acf9a06c672d48ba4c843c 1392 1391 2013-05-23T21:28:25Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK 2e30e8399ce7df6d85f08d89c0643ea5a526d806 1393 1392 2013-05-24T10:39:41Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France cd25ff0241add0c5da7207d0a581b58db95e7cd4 1394 1393 2013-05-24T23:23:59Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia af0ab67d5a0468d77a6e835edc0d5b994fa581f2 1395 1394 2013-05-25T20:15:31Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK 7c3c13813b5326f47c8aef6d169f9e2d01e3e548 1397 1395 2013-05-27T08:25:39Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Delchambre Ludovic, University of Liège, Belgium e1f40fd15608d6b40dfb8cc426eaed35560e4cbe 1398 1397 2013-05-27T08:35:57Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 30 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium b09027f92bd8359dc33085781f08dcad982bc967 1399 1398 2013-05-27T08:36:20Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium 5f3ccd8f549ce6a7a1739494b1a4aaeb01a9e8ff 1400 1399 2013-05-27T20:15:28Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy 93334458b3c845c01ce21eac486dec331ab61951 1401 1400 2013-05-28T16:17:29Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK 4e15b8d01c629e284ec040cc1268a06ae79e2526 0 209 1361 2013-05-06T12:16:09Z Lukasz 2 Created page with "==Venue == '''The conference will be held in the IAP amphitheatre''' Address : 98 bis boulevard Arago, 75014 Paris, France Metro : Denfert Rochereau and St Jacques, line 6 and ..." wikitext text/x-wiki ==Venue == '''The conference will be held in the IAP amphitheatre''' Address : 98 bis boulevard Arago, 75014 Paris, France Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. 7002e4980235047948cc526dc0794b0d59c17eb4 1362 1361 2013-05-06T12:16:16Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the IAP amphitheatre''' Address : 98 bis boulevard Arago, 75014 Paris, France Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. 30af76b4955f87c4bc2ae865cbf687b900d56f46 1363 1362 2013-05-06T12:16:30Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the IAP amphitheatre''' Address : 98 bis boulevard Arago, 75014 Paris, France Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. 7002e4980235047948cc526dc0794b0d59c17eb4 1364 1363 2013-05-06T12:16:46Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the IAP amphitheatre''' Address : 98 bis boulevard Arago, 75014 Paris, France Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. 38c08efdddccdd62af6a0b45f57190a62708af67 1365 1364 2013-05-06T12:17:30Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. a61eb7ff858d1b9b6c5bb6707277150a45557d33 1366 1365 2013-05-06T12:19:06Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. bc289aa2eed2f56c90cf9272b87b1fc8232f16d6 1367 1366 2013-05-06T12:19:52Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. <li>Hotel (★)</li> 7d2d5e82b8522d1bf95ff933ae1d74107ce9a26e 1368 1367 2013-05-06T12:20:28Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotel (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b><a href="http://www.youngandhappy.fr/" target="_blank">YOUNG AND HAPPY HOSTEL</a></b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> 305d0f8725ad7e08494ee805815d63210fd2e16d 1369 1368 2013-05-06T12:20:43Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotel (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b><a href="http://www.youngandhappy.fr/"</a></b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> caa3fe82750c95da5b4a56b7795331a910b582e5 1370 1369 2013-05-06T12:20:55Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotel (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b><a href="http://www.youngandhappy.fr/"</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> 7473751c3720733dff74038d88f5978ebee0b8d8 1371 1370 2013-05-06T12:21:25Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotel (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> 1f38db113b366809a5a1fd96ca56cc68df14a226 1372 1371 2013-05-06T12:23:12Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotel (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <li>Hotel (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait� - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> 3d456c69419c8bd69f65626fd41b582e62510b3c 1373 1372 2013-05-06T12:27:29Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotel (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <li>Hotel (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> <li>Hotel (★★★) <p><b>[http://www.midi-hotel-paris.com/english/" HOTEL du MIDI]</b> (5 min walk)<br> Address: 4, Avenue René Coty, 75014 Paris<br> Tel: 33 (0)1 43 27 23 25</p> <p><b>[http://www.hotel-aramis.com/" HOTEL ARAMIS SAINT-GERMAIN (BEST WESTERN)]</b> (Metro: Saint-Placide / Rennes - direct Bus: 68)<br> Address: 124, rue de Rennes, 75006 Paris<br> Tel: 33 (0)1 45 48 03 75</p> <p><b>[http://www.mercure.com/gb/hotel-1969-mercure-paris-gobelins-place-d-italie/index.shtml" HOTEL MERCURE PARIS GOBELINS PLACE D'ITALIE]</b> (Metro: Place d'Italie)<br> Address: 8 bis avenue de la Soeur Rosalie, 75013 Paris<br> Tel: 33 (0)1 43 36 62 00</p> <p><b>[http://www.hotel-novanox.com/english/index.htm HOTEL NOVANOX]</b> (Metro: Raspail - RER B: Port Royal - Bus: 38)<br> Address: 155, boulevard du Montparnasse, 75014 Paris<br> Tel: 33 (0)1 46 33 63 60</p> <p><b>[http://www.observatoirehotel.com/en/index/ HOTEL OBSERVATOIRE-LUXEMBOURG]</b> (RER B: Luxembourg, or 10 min walk, or Bus: 38)<br> Address: 107, boulevard Saint-Michel, 75005 Paris<br> Tel: 33 (0)1 46 34 10 12</p> <p><b>[http://www.hotelsophiegermain.com HOTEL SOPHIE GERMAIN]</b> (10 min walk)<br> Address: 12, rue Sophie Germain, 75014 Paris<br> Tel: 33 (0)1 43 21 43 75</p> <p><b>[http://www.hotels-la-tour.com/" HOTEL LA TOUR NOTRE-DAME]</b> (Metro/RER B and C: Saint-Michel - Notre-Dame - Bus: 38)<br> Address: 20, rue du Sommerard, 75005 Paris<br> Tel: 33 (0)1 43 54 47 60</p> <li>Hotel (★★★★) <p><b>[http://en.kkhotels.com/hotels/paris/paris/welcome/ K+K HOTEL CAYRE]</b> (Metro: Rue du Bac - direct Bus: 68)<br> Address: 4, boulevard Raspail, 75007 Paris<br> Tel: 33 (0)1 45 44 38 88</p> <p><b>[http://www.parismarriottrivegauche.com/ PARIS MARRIOTT RIVE GAUCHE HOTEL]</b> (10 min walk)<br> Address: 17, boulevard Saint-Jacques, 75014 Paris<br> Tel: 33 (0)1 40 78 79 80</p> c3ec6fb304cb3837d997d3861169b69c15f85ad7 1374 1373 2013-05-06T12:28:03Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotels (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <li>Hotels (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> <li>Hotels (★★★) <p><b>[http://www.midi-hotel-paris.com/english/" HOTEL du MIDI]</b> (5 min walk)<br> Address: 4, Avenue René Coty, 75014 Paris<br> Tel: 33 (0)1 43 27 23 25</p> <p><b>[http://www.hotel-aramis.com/" HOTEL ARAMIS SAINT-GERMAIN (BEST WESTERN)]</b> (Metro: Saint-Placide / Rennes - direct Bus: 68)<br> Address: 124, rue de Rennes, 75006 Paris<br> Tel: 33 (0)1 45 48 03 75</p> <p><b>[http://www.mercure.com/gb/hotel-1969-mercure-paris-gobelins-place-d-italie/index.shtml" HOTEL MERCURE PARIS GOBELINS PLACE D'ITALIE]</b> (Metro: Place d'Italie)<br> Address: 8 bis avenue de la Soeur Rosalie, 75013 Paris<br> Tel: 33 (0)1 43 36 62 00</p> <p><b>[http://www.hotel-novanox.com/english/index.htm HOTEL NOVANOX]</b> (Metro: Raspail - RER B: Port Royal - Bus: 38)<br> Address: 155, boulevard du Montparnasse, 75014 Paris<br> Tel: 33 (0)1 46 33 63 60</p> <p><b>[http://www.observatoirehotel.com/en/index/ HOTEL OBSERVATOIRE-LUXEMBOURG]</b> (RER B: Luxembourg, or 10 min walk, or Bus: 38)<br> Address: 107, boulevard Saint-Michel, 75005 Paris<br> Tel: 33 (0)1 46 34 10 12</p> <p><b>[http://www.hotelsophiegermain.com HOTEL SOPHIE GERMAIN]</b> (10 min walk)<br> Address: 12, rue Sophie Germain, 75014 Paris<br> Tel: 33 (0)1 43 21 43 75</p> <p><b>[http://www.hotels-la-tour.com/" HOTEL LA TOUR NOTRE-DAME]</b> (Metro/RER B and C: Saint-Michel - Notre-Dame - Bus: 38)<br> Address: 20, rue du Sommerard, 75005 Paris<br> Tel: 33 (0)1 43 54 47 60</p> <li>Hotels (★★★★) <p><b>[http://en.kkhotels.com/hotels/paris/paris/welcome/ K+K HOTEL CAYRE]</b> (Metro: Rue du Bac - direct Bus: 68)<br> Address: 4, boulevard Raspail, 75007 Paris<br> Tel: 33 (0)1 45 44 38 88</p> <p><b>[http://www.parismarriottrivegauche.com/ PARIS MARRIOTT RIVE GAUCHE HOTEL]</b> (10 min walk)<br> Address: 17, boulevard Saint-Jacques, 75014 Paris<br> Tel: 33 (0)1 40 78 79 80</p> 565db627d33c803cc730d152f3bb4418cf952909 1375 1374 2013-05-06T12:28:24Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotels (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <div><li>Hotels (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> <li>Hotels (★★★) <p><b>[http://www.midi-hotel-paris.com/english/" HOTEL du MIDI]</b> (5 min walk)<br> Address: 4, Avenue René Coty, 75014 Paris<br> Tel: 33 (0)1 43 27 23 25</p> <p><b>[http://www.hotel-aramis.com/" HOTEL ARAMIS SAINT-GERMAIN (BEST WESTERN)]</b> (Metro: Saint-Placide / Rennes - direct Bus: 68)<br> Address: 124, rue de Rennes, 75006 Paris<br> Tel: 33 (0)1 45 48 03 75</p> <p><b>[http://www.mercure.com/gb/hotel-1969-mercure-paris-gobelins-place-d-italie/index.shtml" HOTEL MERCURE PARIS GOBELINS PLACE D'ITALIE]</b> (Metro: Place d'Italie)<br> Address: 8 bis avenue de la Soeur Rosalie, 75013 Paris<br> Tel: 33 (0)1 43 36 62 00</p> <p><b>[http://www.hotel-novanox.com/english/index.htm HOTEL NOVANOX]</b> (Metro: Raspail - RER B: Port Royal - Bus: 38)<br> Address: 155, boulevard du Montparnasse, 75014 Paris<br> Tel: 33 (0)1 46 33 63 60</p> <p><b>[http://www.observatoirehotel.com/en/index/ HOTEL OBSERVATOIRE-LUXEMBOURG]</b> (RER B: Luxembourg, or 10 min walk, or Bus: 38)<br> Address: 107, boulevard Saint-Michel, 75005 Paris<br> Tel: 33 (0)1 46 34 10 12</p> <p><b>[http://www.hotelsophiegermain.com HOTEL SOPHIE GERMAIN]</b> (10 min walk)<br> Address: 12, rue Sophie Germain, 75014 Paris<br> Tel: 33 (0)1 43 21 43 75</p> <p><b>[http://www.hotels-la-tour.com/" HOTEL LA TOUR NOTRE-DAME]</b> (Metro/RER B and C: Saint-Michel - Notre-Dame - Bus: 38)<br> Address: 20, rue du Sommerard, 75005 Paris<br> Tel: 33 (0)1 43 54 47 60</p> <li>Hotels (★★★★) <p><b>[http://en.kkhotels.com/hotels/paris/paris/welcome/ K+K HOTEL CAYRE]</b> (Metro: Rue du Bac - direct Bus: 68)<br> Address: 4, boulevard Raspail, 75007 Paris<br> Tel: 33 (0)1 45 44 38 88</p> <p><b>[http://www.parismarriottrivegauche.com/ PARIS MARRIOTT RIVE GAUCHE HOTEL]</b> (10 min walk)<br> Address: 17, boulevard Saint-Jacques, 75014 Paris<br> Tel: 33 (0)1 40 78 79 80</p> 16b038c06fb38f72f46b6c5fe5713e4302a2647d 1376 1375 2013-05-06T12:28:33Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotels (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <hr><li>Hotels (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> <li>Hotels (★★★) <p><b>[http://www.midi-hotel-paris.com/english/" HOTEL du MIDI]</b> (5 min walk)<br> Address: 4, Avenue René Coty, 75014 Paris<br> Tel: 33 (0)1 43 27 23 25</p> <p><b>[http://www.hotel-aramis.com/" HOTEL ARAMIS SAINT-GERMAIN (BEST WESTERN)]</b> (Metro: Saint-Placide / Rennes - direct Bus: 68)<br> Address: 124, rue de Rennes, 75006 Paris<br> Tel: 33 (0)1 45 48 03 75</p> <p><b>[http://www.mercure.com/gb/hotel-1969-mercure-paris-gobelins-place-d-italie/index.shtml" HOTEL MERCURE PARIS GOBELINS PLACE D'ITALIE]</b> (Metro: Place d'Italie)<br> Address: 8 bis avenue de la Soeur Rosalie, 75013 Paris<br> Tel: 33 (0)1 43 36 62 00</p> <p><b>[http://www.hotel-novanox.com/english/index.htm HOTEL NOVANOX]</b> (Metro: Raspail - RER B: Port Royal - Bus: 38)<br> Address: 155, boulevard du Montparnasse, 75014 Paris<br> Tel: 33 (0)1 46 33 63 60</p> <p><b>[http://www.observatoirehotel.com/en/index/ HOTEL OBSERVATOIRE-LUXEMBOURG]</b> (RER B: Luxembourg, or 10 min walk, or Bus: 38)<br> Address: 107, boulevard Saint-Michel, 75005 Paris<br> Tel: 33 (0)1 46 34 10 12</p> <p><b>[http://www.hotelsophiegermain.com HOTEL SOPHIE GERMAIN]</b> (10 min walk)<br> Address: 12, rue Sophie Germain, 75014 Paris<br> Tel: 33 (0)1 43 21 43 75</p> <p><b>[http://www.hotels-la-tour.com/" HOTEL LA TOUR NOTRE-DAME]</b> (Metro/RER B and C: Saint-Michel - Notre-Dame - Bus: 38)<br> Address: 20, rue du Sommerard, 75005 Paris<br> Tel: 33 (0)1 43 54 47 60</p> <li>Hotels (★★★★) <p><b>[http://en.kkhotels.com/hotels/paris/paris/welcome/ K+K HOTEL CAYRE]</b> (Metro: Rue du Bac - direct Bus: 68)<br> Address: 4, boulevard Raspail, 75007 Paris<br> Tel: 33 (0)1 45 44 38 88</p> <p><b>[http://www.parismarriottrivegauche.com/ PARIS MARRIOTT RIVE GAUCHE HOTEL]</b> (10 min walk)<br> Address: 17, boulevard Saint-Jacques, 75014 Paris<br> Tel: 33 (0)1 40 78 79 80</p> ce85cf673500ce90bfbb541ab189f3ab685daed5 1377 1376 2013-05-06T12:28:46Z Lukasz 2 /* Accommodation */ wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Accommodation == <li>Hotels (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <li>Hotels (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> <li>Hotels (★★★) <p><b>[http://www.midi-hotel-paris.com/english/" HOTEL du MIDI]</b> (5 min walk)<br> Address: 4, Avenue René Coty, 75014 Paris<br> Tel: 33 (0)1 43 27 23 25</p> <p><b>[http://www.hotel-aramis.com/" HOTEL ARAMIS SAINT-GERMAIN (BEST WESTERN)]</b> (Metro: Saint-Placide / Rennes - direct Bus: 68)<br> Address: 124, rue de Rennes, 75006 Paris<br> Tel: 33 (0)1 45 48 03 75</p> <p><b>[http://www.mercure.com/gb/hotel-1969-mercure-paris-gobelins-place-d-italie/index.shtml" HOTEL MERCURE PARIS GOBELINS PLACE D'ITALIE]</b> (Metro: Place d'Italie)<br> Address: 8 bis avenue de la Soeur Rosalie, 75013 Paris<br> Tel: 33 (0)1 43 36 62 00</p> <p><b>[http://www.hotel-novanox.com/english/index.htm HOTEL NOVANOX]</b> (Metro: Raspail - RER B: Port Royal - Bus: 38)<br> Address: 155, boulevard du Montparnasse, 75014 Paris<br> Tel: 33 (0)1 46 33 63 60</p> <p><b>[http://www.observatoirehotel.com/en/index/ HOTEL OBSERVATOIRE-LUXEMBOURG]</b> (RER B: Luxembourg, or 10 min walk, or Bus: 38)<br> Address: 107, boulevard Saint-Michel, 75005 Paris<br> Tel: 33 (0)1 46 34 10 12</p> <p><b>[http://www.hotelsophiegermain.com HOTEL SOPHIE GERMAIN]</b> (10 min walk)<br> Address: 12, rue Sophie Germain, 75014 Paris<br> Tel: 33 (0)1 43 21 43 75</p> <p><b>[http://www.hotels-la-tour.com/" HOTEL LA TOUR NOTRE-DAME]</b> (Metro/RER B and C: Saint-Michel - Notre-Dame - Bus: 38)<br> Address: 20, rue du Sommerard, 75005 Paris<br> Tel: 33 (0)1 43 54 47 60</p> <li>Hotels (★★★★) <p><b>[http://en.kkhotels.com/hotels/paris/paris/welcome/ K+K HOTEL CAYRE]</b> (Metro: Rue du Bac - direct Bus: 68)<br> Address: 4, boulevard Raspail, 75007 Paris<br> Tel: 33 (0)1 45 44 38 88</p> <p><b>[http://www.parismarriottrivegauche.com/ PARIS MARRIOTT RIVE GAUCHE HOTEL]</b> (10 min walk)<br> Address: 17, boulevard Saint-Jacques, 75014 Paris<br> Tel: 33 (0)1 40 78 79 80</p> 747d427f15b8388b178deef6c5c5d0b96b31fbbd 1378 1377 2013-05-06T12:30:18Z Lukasz 2 wikitext text/x-wiki ==Venue == '''The conference will be held in the [http://www.iap.fr/ IAP]''' Address : 98 bis boulevard Arago, 75014 Paris, France, [http://goo.gl/maps/mRDnt Google Maps] Metro : Denfert Rochereau and St Jacques, line 6 and line 4 RER B : Denfert Rochereau == How to reach IAP == * '''From the airport Roissy Charles de Gaulle''': Take RER B southbound - Denfert Rochereau (via Paris). Or Air France bus to Denfert-Rochereau. Duration: 1 hour. * '''From the Orly airport''' Take the underground automated Orlyval until Antony, then take the RER B to Gare du Nord to Denfert-Rochereau. Duration: 40 min. Or take the bus Orlybus to Denfert-Rochereau. Duration: 35 min * '''From the Gare du Nord''' Take the RER B southbound - Denfert Rochereau (via Paris) or line 4 direction Porte d'Orléans, Denfert Rochereau. Duration: 30 min. * '''From the Gare de Lyon''' Take metro line 14, change at Bercy to line 6, direction Charles de Gaulle - Etoile and get off at St Jacques. Duration: 20 min. == Restaurants == [http://goo.gl/maps/bLWO This map] shows restaurants near the IAP and in Montparnasse Some may be more suitable for an evening meals than lunch. == Accommodation == <li>Hotels (★) <p><b>HOTEL DE L'ESPERANCE</b> (5 min walk)<br> Address: 1, rue Grancey 75014 Paris<br> Tel: 33 (0)1 43 21 41 04</p> <p><b>HOTEL FORMULE 1</b> (Metro: PORTE D'ORLEANS + 10 min walk)<br> Address: 23, av. Porte de Chatillon 75014 PARIS<br> Tel: 08 91 70 52 29</p> <p><b>[http://www.youngandhappy.fr/ Young And Happy]</b> (Place Monge / 20 min walk)<br> Address: 80, rue Mouffetard 75005 PARIS<br> Tel: 01 47 07 47 07</p> <li>Hotels (★★) <p><b>[http://www.paris-hotel-lion.com HOTEL DU LION]</b> (5 min walk)<br> Address: 1, avenue du Général leclerc 75014 Paris<br> Tel: 33 (1) 40 47 04 00</p> <p><b>[http://www.agenor-paris-hotel.com HOTEL AGENOR]</b> (Metro: Gait - 10 min walk)<br> Address: 22, rue Cels 75014 Paris<br> Tel: 33 (0)1 43 22 47 25</p> <p><b>HOTEL LE LIONCEAU / HOTEL DES VOYAGEURS</b> (5 min walk)<br> Address: 22, rue Daguerre / 22 rue Boulard 75014 Paris<br> Tel: 33 (0)1 43 22 53 53 </p> <p><b>[http://www.hotel-moulinvert.com/ HOTEL du MOULIN VERT]</b> (Metro: Pernety / Alésia - direct Bus: 38)<br> Address: 74, rue du Moulin Vert 75014 Paris<br> Tel: 33 (0)1 45 43 65 38</p> <p><b>[http://www.hotelduparc-paris.com HOTEL DU PARC]</b> (Metro: Edgar-Quinet - Montparnasse)<br> Address: 6, rue Jolivet, 75014 Paris<br> Tel: 33 (0)1 43 20 95 54</p> <p><b>[http://www.hotelkyriadparis.com HOTEL KYRIAD Italie-Gobelins]</b> (Metro: Place d'Italie, Bus: 83 + 38)<br> Address: 5 rue Véronèse, 75013 PARIS<br> Tel: 33 (0)1 47 07 20 90</p> <li>Hotels (★★★) <p><b>[http://www.midi-hotel-paris.com/english/" HOTEL du MIDI]</b> (5 min walk)<br> Address: 4, Avenue René Coty, 75014 Paris<br> Tel: 33 (0)1 43 27 23 25</p> <p><b>[http://www.hotel-aramis.com/" HOTEL ARAMIS SAINT-GERMAIN (BEST WESTERN)]</b> (Metro: Saint-Placide / Rennes - direct Bus: 68)<br> Address: 124, rue de Rennes, 75006 Paris<br> Tel: 33 (0)1 45 48 03 75</p> <p><b>[http://www.mercure.com/gb/hotel-1969-mercure-paris-gobelins-place-d-italie/index.shtml" HOTEL MERCURE PARIS GOBELINS PLACE D'ITALIE]</b> (Metro: Place d'Italie)<br> Address: 8 bis avenue de la Soeur Rosalie, 75013 Paris<br> Tel: 33 (0)1 43 36 62 00</p> <p><b>[http://www.hotel-novanox.com/english/index.htm HOTEL NOVANOX]</b> (Metro: Raspail - RER B: Port Royal - Bus: 38)<br> Address: 155, boulevard du Montparnasse, 75014 Paris<br> Tel: 33 (0)1 46 33 63 60</p> <p><b>[http://www.observatoirehotel.com/en/index/ HOTEL OBSERVATOIRE-LUXEMBOURG]</b> (RER B: Luxembourg, or 10 min walk, or Bus: 38)<br> Address: 107, boulevard Saint-Michel, 75005 Paris<br> Tel: 33 (0)1 46 34 10 12</p> <p><b>[http://www.hotelsophiegermain.com HOTEL SOPHIE GERMAIN]</b> (10 min walk)<br> Address: 12, rue Sophie Germain, 75014 Paris<br> Tel: 33 (0)1 43 21 43 75</p> <p><b>[http://www.hotels-la-tour.com/" HOTEL LA TOUR NOTRE-DAME]</b> (Metro/RER B and C: Saint-Michel - Notre-Dame - Bus: 38)<br> Address: 20, rue du Sommerard, 75005 Paris<br> Tel: 33 (0)1 43 54 47 60</p> <li>Hotels (★★★★) <p><b>[http://en.kkhotels.com/hotels/paris/paris/welcome/ K+K HOTEL CAYRE]</b> (Metro: Rue du Bac - direct Bus: 68)<br> Address: 4, boulevard Raspail, 75007 Paris<br> Tel: 33 (0)1 45 44 38 88</p> <p><b>[http://www.parismarriottrivegauche.com/ PARIS MARRIOTT RIVE GAUCHE HOTEL]</b> (10 min walk)<br> Address: 17, boulevard Saint-Jacques, 75014 Paris<br> Tel: 33 (0)1 40 78 79 80</p> a1bd51b92bce81c2d0eccf00bde05bfb3f880abc 0 204 1379 1337 2013-05-06T12:31:37Z Lukasz 2 /* Workshop Organizing Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop will be held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics this year include: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda]] * [[workshop2013:registration|Registration]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore * Iain Steele b385468c9508a4c7d36fc87aacd74644ae80519a 0 206 1396 1345 2013-05-25T20:16:36Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiasciencealertsworkshop2013@gmail.com'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Thursday 20th''''' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} a68a177134e6b457a2bb32006890d32cbe68d7c7 0 205 1402 1401 2013-05-29T12:26:17Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France 65443a9b162f4bf7f3d8f136bf14332e9937135a 1403 1402 2013-05-29T14:50:19Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria 4097d8a83a5ad0c68ee47d4342a106ceca30e1e0 1404 1403 2013-05-30T19:50:28Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland f275ceb0d4f8b35e2be1bc118b18310a8817b1c7 1405 1404 2013-05-31T10:52:28Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK ade5f31ea3b39af8bb7db454b660ec6480c56ea8 1406 1405 2013-05-31T11:12:25Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK f72c96dd13656bbadabd7aa84153d73d783dce34 1407 1406 2013-05-31T13:50:59Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA 66d91e5bd631188d077b8cf0200d415bfd1c580f 1408 1407 2013-05-31T18:44:02Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland 787718b0e70a27492adc63928c69cb359fdbf6da 1409 1408 2013-06-02T21:33:49Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # George Seabroke, MSSL, UCL, UK dc8d4cd2e3b65893628bbf8ce5ba8768dccf979c 1412 1409 2013-06-03T14:15:45Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # George Seabroke, MSSL, UCL, UK # Jean-Baptiste Marquette, IAP, France 1b5ef2c0f0a4f15c61ddf6d0c49d3e18b1985e7c 1413 1412 2013-06-04T09:07:07Z Lukasz 2 wikitext text/x-wiki <big>'''Please register here: [[Workshop2013:registrationform | Registration form]]</big> ''' '''Registration closes on 31 May 2013''' ---- List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # George Seabroke, MSSL, UCL, UK # Jean-Baptiste Marquette, IAP, France # Roger Ferlet, IAP, France # Daniel Hestroffer, IMCEE, France # Christine Ducourant, Laboratoire d'Astrophysique de Bordeaux, France 12f977c3044c52e4fb1123118345aef741b375b9 1416 1413 2013-06-08T22:20:30Z Lukasz 2 wikitext text/x-wiki List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Tim Staley, University of Southampton, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # George Seabroke, MSSL, UCL, UK # Jean-Baptiste Marquette, IAP, France # Roger Ferlet, IAP, France # Daniel Hestroffer, IMCEE, France # Christine Ducourant, Laboratoire d'Astrophysique de Bordeaux, France f94dc7f5856b1ed7683c068263887fe763379335 1417 1416 2013-06-10T10:44:06Z Lukasz 2 wikitext text/x-wiki List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # George Seabroke, MSSL, UCL, UK # Jean-Baptiste Marquette, IAP, France # Roger Ferlet, IAP, France # Daniel Hestroffer, IMCEE, France # Christine Ducourant, Laboratoire d'Astrophysique de Bordeaux, France # Michel Dennefeld, IAP, France d60f81fe32be2a1c786d7aab2e3e1c843f858cc0 1427 1417 2013-06-12T20:49:23Z Lukasz 2 wikitext text/x-wiki List of registered participants: # Peter Jonker, SRON, Netherlands # Laszlo Szabados, Konkoly Observatory, Hungary # Krisztián Vida, MTA CSFK CSI, Hungary # Irek Khamitov, Tubitak National Observatory, Turkey # Pavel Koubsky, Ondrejov Observatory, Czech Rep. # Norbert Schartel, XMM-Newton, ESA # Mark Sullivan, Southampton, PESSTO, UK # Paolo Tanga, Observatoire de la Côte d'Azur, France # John Davies, UKATC, Royal Observatory, Edinburgh, UK # Jon Marchant, Liverpool John Moores University, UK # Helene Sol, CNRS, Observatoire de Paris, France # Simon Hodgkin, IoA, Cambridge, UK # Nicholas Walton, IoA, Cambridge, UK # Stephen Potter, South African Astronomical Observatory # Chris Davis, Liverpool Telescope/Liverpool JMU, UK # Shay Zucker, Tel Aviv University, Israel # Stuart Littlefair, University of Sheffield, UK # Liam Hardy, University of Sheffield, UK # Ashish Mahabal, Caltech, USA # Phillipe Bendjoya, UNS-OCA-CNRS, France # Gerry Gilmore, IoA, Cambridge, UK # Heather Campbell, IoA, Cambridge, UK # Olga Suarez, Observatoire de la Cote d'Azur, Nice, France # Evgeny Gorovskoy, Sternberg Astronomical Institute of Lomonosov Moscow University, Russia # Ulrich Kolb, The Open University, UK # Ludovic Delchambre, University of Liège, Belgium # Massimo Turatto, Osservatorio Astronomico di Padova, Italy # Stephen Ridgway, NOAO, USA # Martin Dominik, SUPA, University of St Andrews, UK # Kailash Sahu, Space Telescope Science Institute, USA # Paola Di Matteo, Observatoire de Paris, France # Werner Zeilinger, University of Vienna, Austria # Sjoert van Velzen, Radboud University Nijmegen, The Netherlands # Goran Damljanovic, Astronomical Observatory, Belgrade, Serbia # Dan Maoz, Tel-Aviv University, Israel # Zbigniew Kolaczkowski, Instytut Astronomiczny Uniwersytetu Wrocławskiego, Poland # Fraser Lewis, Faulkes Telescope Project, University of South Wales, UK # Elme Breedt, University of Warwick, UK # Timo Prusti, ESA # William Thuillot, IMCCE-Paris Observatory, France # Krzysztof Ulaczyk, Warsaw University Astronomical Observatory, Poland # Krzysztof Rybicki, Warsaw University Astronomical Observatory, Poland # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # George Seabroke, MSSL, UCL, UK # Jean-Baptiste Marquette, IAP, France # Roger Ferlet, IAP, France # Daniel Hestroffer, IMCEE, France # Christine Ducourant, Laboratoire d'Astrophysique de Bordeaux, France # Michel Dennefeld, IAP, France # Andreja Gomboc, University of Ljubljana, Slovenia 31f17f7dc69b277f8e4615aac22835f835964549 0 208 1410 1389 2013-06-03T08:19:58Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Gaia alerts - how they work, what is the expected yield *Supernovae, microlensing, novae, CVs, AGN flares, and other targets for Gaia Alerts *Arrangements for the alerts follow-up and verification campaign in early 2014 *Follow-up strategies *Current/planned multi-wavelength transient surveys, including X-ray channels *Reports from tests on transient follow-up *Presentation of new potential partners for the follow-up network == Draft Agenda == '''Wed 19. June:''' * lunch * welcome and session I * coffee break * session II '''Thu 20.June:''' * session III * coffee break * session IV * lunch (provided by the organizers) * session V * coffee break * session VI * social dinner '''Fri 21.June:''' * session VII * coffee break * session VIII * lunch and end of the workshop d53ed6cc081fab65e285efc35c494836a340facd 1411 1410 2013-06-03T08:23:10Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Gaia alerts - how they work, what is the expected yield *Supernovae, microlensing, novae, CVs, AGN flares, and other targets for Gaia Alerts *Arrangements for the alerts follow-up and verification campaign in early 2014 *Follow-up strategies *How to get involved in Gaia alerts follow-up networks? *Current/planned multi-wavelength transient surveys, including X-ray channels *Reports from tests on transient follow-up *Presentation of new potential partners for the follow-up network == Draft Agenda == '''Wed 19. June:''' * lunch * welcome and session I * coffee break * session II '''Thu 20.June:''' * session III * coffee break * session IV * lunch (provided by the organizers) * session V * coffee break * session VI * social dinner '''Fri 21.June:''' * session VII * coffee break * session VIII * lunch and end of the workshop 3dd00c9547585d682b8c1543958895247b744705 1414 1411 2013-06-07T11:18:05Z Lukasz 2 wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Gaia alerts - how they work, what is the expected yield *Supernovae, microlensing, novae, CVs, AGN flares, and other targets for Gaia Alerts *Arrangements for the alerts follow-up and verification campaign in early 2014 *Follow-up strategies *How to get involved in Gaia alerts follow-up networks? *Current/planned multi-wavelength transient surveys, including X-ray channels *Reports from tests on transient follow-up *Presentation of new potential partners for the follow-up network == Draft Agenda == '''Wed 19. June:''' * lunch * 14:00 welcome and session I * coffee break * session II '''Thu 20.June:''' * session III * coffee break * session IV * lunch (provided by the organizers) * session V * coffee break * session VI * social dinner '''Fri 21.June:''' * session VII * coffee break * session VIII * lunch and end of the workshop at 13:00 7b201667b65243f84b3e2d7bbdcb6ef3e9259d54 1418 1414 2013-06-11T22:03:55Z Lukasz 2 /* Draft Agenda */ wikitext text/x-wiki The topics this year include: *Status of Gaia - year of the launch! *Gaia alerts - how they work, what is the expected yield *Supernovae, microlensing, novae, CVs, AGN flares, and other targets for Gaia Alerts *Arrangements for the alerts follow-up and verification campaign in early 2014 *Follow-up strategies *How to get involved in Gaia alerts follow-up networks? *Current/planned multi-wavelength transient surveys, including X-ray channels *Reports from tests on transient follow-up *Presentation of new potential partners for the follow-up network ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |MD+LW+STH |Welcome |10 |---- |14:10 |Timo Prusti |Gaia status |30 |---- |14:40 |Simon Hodgkin |AlertPipe Status |30 |---- |15:10 |Lukasz Wyrzykowski |Detection and classification in the AlertPipe |30 |---- |15:40 |Nicholas Walton |Automated Classification of Supernovae from Gaia Alerts |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Paola Di Matteo |Spectroscopic science alerts: criteria and implementation |15 |---- |16:45 |George Seabroke |Gaia RVS spectra as follow-up to Photo Science Alerts |15 |---- |17:00 |Paolo Tanga |Solar System alerts |20 |---- |17:20 |Ashish Mahabal |New Measures for Different Transients |30 |---- |17:50 |Stephen Ridgway |Detection rate for variable stars |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Kailash Sahu |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |25 |---- |09:55 |Shay Zucker |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |25 |---- |10:20 |Sjoert van Velzen |Optical searches for stellar tidal disruption flares |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Peter Jonker |Connecting LOFAR radio, X-ray and optical GAIA transients |25 |---- |11:40 |Helene Sol |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |25 |---- |12:05 |Elme Breedt |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |25 |---- |12:30 |Evgeny Gorovskoy |Discovery optical transients on MASTER robotic telescope network. |15 |---- |12:45 |Krisztián Vida |The Fly's Eye camera system |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |John Davies |OPTICON, the Plans for FP7: 2013-2016 |15 |---- |14:15 |Mark Sullivan |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |15 |---- |14:30 |Ulrich Kolb |Science with PIRATE |15 |---- |14:45 |Stuart Littlefair |The pt5m robotic telescope on La Palma |15 |---- |15:00 |Pavel Koubsky |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |15 |---- |15:15 |Werner Zeilinger |Transient astronomy with the observing facilities of the Vienna Observatory |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Simon Hodgkin |Alerts Verification and discussion |60 |---- |17:00 |Irek Khamitov |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |15 |---- |17:15 |Laszlo Szabados |Konkoly Observatory - Observing Facilities and Photometric Projects |15 |---- |17:30 |Goran Damljanovic |The photometric observations of Gaia alerts with 60cm ASV telescope |15 |---- |17:45 |Zbigniew Kołaczkowski |Wroclaw Observatory |15 |---- |18:00 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Chris Davis |Time Domain Astronomy with the Liverpool Telescope |15 |---- |09:45 |Fraser Lewis |Observing with the Faulkes Telescopes |15 |---- |10:00 |Stephen Potter |South African Astronomy and Observatories |15 |---- |10:15 |Massimo Turatto |The Asiago facilities |15 |---- |10:30 |Phillipe Bendjoya |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |15 |---- |10:45 |Olga Suarez |EduCosmos: Participative science for high school students with 1m telescopes |15 |---- |11:00 |Michel Dennefeld et al |Involvement of amateur astronomers |20 |---- |11:20 |'''''Coffee break''''' | |30 |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 80ae66df7f453dde05f0a7b714b11abfd32f0056 1419 1418 2013-06-11T22:04:11Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |MD+LW+STH |Welcome |10 |---- |14:10 |Timo Prusti |Gaia status |30 |---- |14:40 |Simon Hodgkin |AlertPipe Status |30 |---- |15:10 |Lukasz Wyrzykowski |Detection and classification in the AlertPipe |30 |---- |15:40 |Nicholas Walton |Automated Classification of Supernovae from Gaia Alerts |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Paola Di Matteo |Spectroscopic science alerts: criteria and implementation |15 |---- |16:45 |George Seabroke |Gaia RVS spectra as follow-up to Photo Science Alerts |15 |---- |17:00 |Paolo Tanga |Solar System alerts |20 |---- |17:20 |Ashish Mahabal |New Measures for Different Transients |30 |---- |17:50 |Stephen Ridgway |Detection rate for variable stars |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Kailash Sahu |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |25 |---- |09:55 |Shay Zucker |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |25 |---- |10:20 |Sjoert van Velzen |Optical searches for stellar tidal disruption flares |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Peter Jonker |Connecting LOFAR radio, X-ray and optical GAIA transients |25 |---- |11:40 |Helene Sol |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |25 |---- |12:05 |Elme Breedt |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |25 |---- |12:30 |Evgeny Gorovskoy |Discovery optical transients on MASTER robotic telescope network. |15 |---- |12:45 |Krisztián Vida |The Fly's Eye camera system |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |John Davies |OPTICON, the Plans for FP7: 2013-2016 |15 |---- |14:15 |Mark Sullivan |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |15 |---- |14:30 |Ulrich Kolb |Science with PIRATE |15 |---- |14:45 |Stuart Littlefair |The pt5m robotic telescope on La Palma |15 |---- |15:00 |Pavel Koubsky |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |15 |---- |15:15 |Werner Zeilinger |Transient astronomy with the observing facilities of the Vienna Observatory |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Simon Hodgkin |Alerts Verification and discussion |60 |---- |17:00 |Irek Khamitov |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |15 |---- |17:15 |Laszlo Szabados |Konkoly Observatory - Observing Facilities and Photometric Projects |15 |---- |17:30 |Goran Damljanovic |The photometric observations of Gaia alerts with 60cm ASV telescope |15 |---- |17:45 |Zbigniew Kołaczkowski |Wroclaw Observatory |15 |---- |18:00 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Chris Davis |Time Domain Astronomy with the Liverpool Telescope |15 |---- |09:45 |Fraser Lewis |Observing with the Faulkes Telescopes |15 |---- |10:00 |Stephen Potter |South African Astronomy and Observatories |15 |---- |10:15 |Massimo Turatto |The Asiago facilities |15 |---- |10:30 |Phillipe Bendjoya |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |15 |---- |10:45 |Olga Suarez |EduCosmos: Participative science for high school students with 1m telescopes |15 |---- |11:00 |Michel Dennefeld et al |Involvement of amateur astronomers |20 |---- |11:20 |'''''Coffee break''''' | |30 |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 6dfed62bf1042820b8bff2f223c47758fdae4d2d 1420 1419 2013-06-11T22:06:43Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |15 |---- |14:15 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:30 |Science with PIRATE |Ulrich Kolb |15 |---- |14:45 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:00 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:15 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:15 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:30 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |17:45 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:00 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | |30 |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 9324bb19c9f97324e163461eb90768c5201d46a1 1421 1420 2013-06-11T22:07:23Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |15 |---- |14:15 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:30 |Science with PIRATE |Ulrich Kolb |15 |---- |14:45 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:00 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:15 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:15 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:30 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |17:45 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:00 |'''''end of day2''''' | | |---- |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | |30 |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 623d78810026e7ea9e737e899b40020b80a1ff60 1422 1421 2013-06-11T22:07:49Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |15 |---- |14:15 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:30 |Science with PIRATE |Ulrich Kolb |15 |---- |14:45 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:00 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:15 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:15 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:30 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |17:45 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:00 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | |30 |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 9324bb19c9f97324e163461eb90768c5201d46a1 1424 1422 2013-06-11T22:40:10Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |15 |---- |14:15 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:30 |Science with PIRATE |Ulrich Kolb |15 |---- |14:45 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:00 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:15 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:15 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:30 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |17:45 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:00 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | | |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} faba83de21ea90d297e00d02b7b689e9ca11ea7f 1425 1424 2013-06-12T15:14:08Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:30 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | | |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} d547208361daf0e1d2780264e31c48f5ef0aaaa7 1426 1425 2013-06-12T15:14:26Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | | |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} dbe64d82bc743554a3f0e0ebe9f2c71c9d5bbc62 1428 1426 2013-06-12T22:14:11Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[File:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | | |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 29ccb75308ec8fd49c769be02bd98e7fcbed83f4 1430 1428 2013-06-12T22:14:37Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:30 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:45 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |10:00 |South African Astronomy and Observatories |Stephen Potter |15 |---- |10:15 |The Asiago facilities |Massimo Turatto |15 |---- |10:30 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:45 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |11:00 |Involvement of amateur astronomers |Michel Dennefeld et al |20 |---- |11:20 |'''''Coffee break''''' | | |---- |11:50 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} dbe64d82bc743554a3f0e0ebe9f2c71c9d5bbc62 1432 1430 2013-06-17T08:23:56Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Michel Dennefeld et al |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 3313c06c48a1db822c846d0f89e710c06ce70daa 1433 1432 2013-06-18T07:37:11Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |colspan="4"|Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Michel Dennefeld et al |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 8724da1d91a24c133d8880dfdb1a25d24641957a 1434 1433 2013-06-18T07:37:32Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Michel Dennefeld et al |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 3ea6dc432ee07f84dcf3ad484241b17f4562b22d 1435 1434 2013-06-18T07:38:06Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Michel Dennefeld et al |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} b833884b79aaa2025b55ec74444c6c65fe3cfa23 1436 1435 2013-06-18T10:54:37Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} d15da6e9996933c83842b09d42cfa336e6f672b4 1437 1436 2013-06-22T21:37:07Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status |Timo Prusti |30 |---- |14:40 |AlertPipe Status |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} ac3a843bc7a2c79e9c995823fa3803a65133c041 1438 1437 2013-06-22T21:38:40Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimePrusit_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NickWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 6101258f9a6874abbea80746f1e48d9f17231e9b 1439 1438 2013-06-22T21:41:49Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimePrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NickWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} ca6b5377fcc41b1b9fa3b454b8ba172d20055e51 1440 1439 2013-06-22T21:42:00Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimoPrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NickWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 072a7d9bf4d5cb62e29e869e6d3be711c39513f0 1441 1440 2013-06-22T21:42:40Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimoPrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NicWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts |George Seabroke |15 |---- |17:00 |Solar System alerts |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network. |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects |Mark Sullivan |15 |---- |14:40 |Science with PIRATE |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO. |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories |Stephen Potter |15 |---- |09:45 |The Asiago facilities |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 9b5ac87653cb007c837bc1e92e851b59f5d030e5 1444 1441 2013-06-25T09:27:45Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimoPrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NicWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoladiMatteo.pdf pdf] |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GeorgeSeabroke.pdf pdf] |George Seabroke |15 |---- |17:00 |Solar System alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoloTanga.pdf pdf] |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StephenRidgway.pdf pdf] |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KailashSahu.pdf pdf] |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ShayZucker.pdf pdf] |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SjoertvanVelzen.pdf pdf] |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PeterJonker.pdf pdf] |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/HeleneSol.pdf pdf] |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ElmeBreedt.pdf pdf] |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/EvgenyGorovskoy.pdf pdf] |Evgeny Gorovskoy |15 |---- |12:45 |The Fly's Eye camera system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KrisztianVida.pdf pdf] |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/JohnDavies.pdf pdf] |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MarkSullivan.pdf pdf] |Mark Sullivan |15 |---- |14:40 |Science with PIRATE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/UlrichKolb.pdf pdf] |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StuartLittlefair.pdf pdf] |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PavelKoubsky.pdf pdf] |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin-verification.pdf pdf] |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/WernerZeilinger.pdf pdf] |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/IrekKhamitov.pdf pdf] |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LaszloSzabados.pdf pdf] |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GoranDamljanovic.pdf pdf] |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ZbigniewKolaczkowski.pdf pdf] |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ChrisDavis.pdf pdf] |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/FraserLewis.pdf pdf] |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StephenPotter.pdf pdf] |Stephen Potter |15 |---- |09:45 |The Asiago facilities [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MassimoTuratto.pdf pdf] |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PhilipeBendjoya.pdf pdf] |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/OlgaSuarez.pdf pdf] |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} 46a316a2ac726e1516faa25e70af971788664bb1 1445 1444 2013-06-25T09:31:18Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimoPrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NicWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoladiMatteo.pdf pdf] |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GeorgeSeabroke.pdf pdf] |George Seabroke |15 |---- |17:00 |Solar System alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoloTanga.pdf pdf] |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StephenRidgway.pdf pdf] |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KailashSahu.pdf pdf] |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ShayZucker.pdf pdf] |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SjoertvanVelzen.pdf pdf] |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PeterJonker.pdf pdf] |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/HeleneSol.pdf pdf] |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ElmeBreedt.pdf pdf] |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/EvgenyGorbovskoy.pdf pdf] |Evgeny Gorbovskoy |15 |---- |12:45 |The Fly's Eye camera system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KrisztianVida.pdf pdf] |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/JohnDavies.pdf pdf] |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MarkSullivan.pdf pdf] |Mark Sullivan |15 |---- |14:40 |Science with PIRATE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/UlrichKolb.pdf pdf] |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StuartLittlefair.pdf pdf] |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PavelKoubsky.pdf pdf] |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin-Verification.pdf pdf] |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/WernerZeilinger.pdf pdf] |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/IrekKhamitov.pdf pdf] |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LaszloSzabados.pdf pdf] |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GoranDamljanovic.pdf pdf] |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ZbigniewKolaczkowski.pdf pdf] |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ChrisDavis.pdf pdf] |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/FraserLewis.pdf pdf] |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/potter_paris_2013.pdf pdf] |Stephen Potter |15 |---- |09:45 |The Asiago facilities [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MassimoTuratto.pdf pdf] |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PhillipeBendjoya.pdf pdf] |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/OlgaSuarez.pdf pdf] |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} ff801a4e9aea6f85866d7f3c2c5039985789bdd1 1446 1445 2013-06-25T09:33:40Z Lukasz 2 wikitext text/x-wiki ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimoPrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NicWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoladiMatteo.pdf pdf] |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GeorgeSeabroke.pdf pdf] |George Seabroke |15 |---- |17:00 |Solar System alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoloTanga.pdf pdf] |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StephenRidgway.pdf pdf] |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KailashSahu.pdf pdf] |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ShayZucker.pdf pdf] |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SjoertvanVelzen.pdf pdf] |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PeterJonker.pdf pdf] |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/HeleneSol.pdf pdf] |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ElmeBreedt.pdf pdf] |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/EvgenyGorbovskoy.pdf pdf] |Evgeny Gorbovskoy |15 |---- |12:45 |The Fly's Eye camera system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KrisztianVida.pdf pdf] |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/JohnDavies.pdf pdf] |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MarkSullivan.pdf pdf] |Mark Sullivan |15 |---- |14:40 |Science with PIRATE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/UlrichKolb.pdf pdf] |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StuartLittlefair.pdf pdf] |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PavelKoubsky.pdf pdf] |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin-Verification.pdf pdf] |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/WernerZeilinger.pdf pdf] |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/IrekKhamitov.pdf pdf] |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LaszloSzabados.pdf pdf] |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GoranDamljanovic.pdf pdf] |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ZbigniewKolaczkowski.pdf pdf] |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ChrisDavis.pdf pdf] |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/FraserLewis.pdf pdf] |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/potter_paris_2013.pdf pdf] |Stephen Potter |15 |---- |09:45 |The Asiago facilities [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MassimoTuratto.pdf pdf] |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PhillipeBendjoya.pdf pdf] |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/OlgaSuarez.pdf pdf] |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/OlivierThizy-poster.pdf poster pdf] |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} adb262f1e99932aeafccc4e3230b1bd6570b6725 1447 1446 2013-06-25T09:34:39Z Lukasz 2 wikitext text/x-wiki The Agenda now serves as an archive of all presentations. The slides are available in the PDF form and the video/audio recording of the presentation will soon be linked here as well. {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |colspan="4"|'''Wednesday, June 19th''' |---- |14:00 |Welcome |MD+LW+STH |10 |---- |14:10 |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/TimoPrusti_toshow.pdf pdf] |Timo Prusti |30 |---- |14:40 |AlertPipe Status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin.pdf pdf] |Simon Hodgkin |30 |---- |15:10 |Detection and classification in the AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LukaszWyrzykowski.pdf pdf] |Lukasz Wyrzykowski |30 |---- |15:40 |Automated Classification of Supernovae from Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/NicWalton.pdf pdf] |Nicholas Walton |20 |---- |16:00 |'''''Coffee break''''' | | |---- |16:30 |Spectroscopic science alerts: criteria and implementation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoladiMatteo.pdf pdf] |Paola Di Matteo |15 |---- |16:45 |Gaia RVS spectra as follow-up to Photo Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GeorgeSeabroke.pdf pdf] |George Seabroke |15 |---- |17:00 |Solar System alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PaoloTanga.pdf pdf] |Paolo Tanga |20 |---- |17:20 |New Measures for Different Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/AshishMahabal.pdf pdf] |Ashish Mahabal |30 |---- |17:50 |Detection rate for variable stars [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StephenRidgway.pdf pdf] |Stephen Ridgway |20 |---- |18:10 |'''''end of day1''''' | | |---- |colspan="4"|'''Thursday, June 20th''' |---- |09:30 |Upcoming Microlensing by Proxima Centauri: A Rare Opportunity for Mass Determination and Planet Detection [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KailashSahu.pdf pdf] |Kailash Sahu |25 |---- |09:55 |Directed Follow-Up strategy - using Gaia Science Alerts to detect transiting Exoplanets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ShayZucker.pdf pdf] |Shay Zucker |25 |---- |10:20 |Optical searches for stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SjoertvanVelzen.pdf pdf] |Sjoert van Velzen |25 |---- |10:45 |'''''Coffee break''''' | |30 |---- |11:15 |Connecting LOFAR radio, X-ray and optical GAIA transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PeterJonker.pdf pdf] |Peter Jonker |25 |---- |11:40 |GAIA alerts on AGN flares: which synergy with observations at Very High Energies ? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/HeleneSol.pdf pdf] |Helene Sol |25 |---- |12:05 |A large, deep, and homogeneous sample of cataclysmic variables from GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ElmeBreedt.pdf pdf] |Elme Breedt |25 |---- |12:30 |Discovery optical transients on MASTER robotic telescope network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/EvgenyGorbovskoy.pdf pdf] |Evgeny Gorbovskoy |15 |---- |12:45 |The Fly's Eye camera system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/KrisztianVida.pdf pdf] |Krisztian Vida |15 |---- |13:00 |'''''Lunch''''' | | |---- |14:00 |OPTICON, the Plans for FP7: 2013-2016 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/JohnDavies.pdf pdf] |John Davies |25 |---- |14:25 |PESSTO: The Public ESO Spectroscopic Survey for Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MarkSullivan.pdf pdf] |Mark Sullivan |15 |---- |14:40 |Science with PIRATE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/UlrichKolb.pdf pdf] |Ulrich Kolb |15 |---- |14:55 |The pt5m robotic telescope on La Palma [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/StuartLittlefair.pdf pdf] |Stuart Littlefair |15 |---- |15:10 |The use of Danish 154 Telescope and DFOSC photometer to follow up the objects from Gaia Alerts project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PavelKoubsky.pdf pdf] |Pavel Koubsky |15 |---- |15:25 |'''''Coffee break''''' | | |---- |16:00 |Alerts Verification and discussion [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/SimonHodgkin-Verification.pdf pdf] |Simon Hodgkin |60 |---- |17:00 |Transient astronomy with the observing facilities of the Vienna Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/WernerZeilinger.pdf pdf] |Werner Zeilinger |15 |---- |17:15 |Observations of PHA 99942 Apophis at RTT150 in frame of Gaia-FUN-SSO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/IrekKhamitov.pdf pdf] |Irek Khamitov |15 |---- |17:30 |Konkoly Observatory - Observing Facilities and Photometric Projects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/LaszloSzabados.pdf pdf] |Laszlo Szabados |15 |---- |17:45 |The photometric observations of Gaia alerts with 60cm ASV telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/GoranDamljanovic.pdf pdf] |Goran Damljanovic |15 |---- |18:00 |Wroclaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ZbigniewKolaczkowski.pdf pdf] |Zbigniew Kołaczkowski |15 |---- |18:15 |'''''end of day2''''' | | |---- |19:30 |colspan="3"|''Workshop Dinner, [http://www.pagesjaunes.fr/trouverlesprofessionnels/ficheDetaillee/plan.do?idBlocAnnonceur=014539313100000000C0001&indexInscriptionSelectionnee=0 Restaurant "Le Moulin Vert", 33 rue du Moulin Vert''] |---- |colspan="4"|'''Friday, June 21th''' |---- |09:00 |Time Domain Astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/ChrisDavis.pdf pdf] |Chris Davis |15 |---- |09:15 |Observing with the Faulkes Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/FraserLewis.pdf pdf] |Fraser Lewis |15 |---- |09:30 |South African Astronomy and Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/potter_paris_2013.pdf pdf] |Stephen Potter |15 |---- |09:45 |The Asiago facilities [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/MassimoTuratto.pdf pdf] |Massimo Turatto |15 |---- |10:00 |The C2PU (Centre Pedagogy Planet Univers) at OCA (Observatoire de la Côte d Azur) in the framework of GAIA-FUN [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/PhillipeBendjoya.pdf pdf] |Phillipe Bendjoya |15 |---- |10:15 |EduCosmos: Participative science for high school students with 1m telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/OlgaSuarez.pdf pdf] |Olga Suarez |15 |---- |10:30 |Involvement of amateur astronomers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2013/slides/OlivierThizy-poster.pdf poster pdf] |Discussion |25 |---- |10:55 |'''''Coffee break''''' | | |---- |11:30 |Discussion and summary | | |---- |13:00 |'''''end of day3''''' | | |---- |} ---- '''Abstract Book is available [[Media:AbstractBook2012.pdf|here]].''' ---- 4c6ca15906daa0bbd87153086d6cc9f057bddc6a 0 204 1415 1379 2013-06-08T22:19:51Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop will be held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics this year include: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda]] * [[workshop2013:registration|Participants]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore * Iain Steele 984998ad630be929080a3a1eb63617ae38240da0 1449 1415 2013-06-25T09:37:11Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop was held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics included: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invited all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda - archive of presentations]] * [[workshop2013:registration|Participants]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore * Iain Steele 87411f68b0645e3a46b7d646fa8db5152ca713ba 1451 1449 2013-06-26T17:15:21Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop was held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics included: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invited all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda - archive of presentations]] * [[workshop2013:registration|Participants]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore * Iain Steele ---- Workshop Photo [[File:photo2013.jpg]] 450deb1b33a2f006023d5a300eed3a316dcb7c2d 6 210 1423 2013-06-11T22:39:18Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1429 1423 2013-06-12T22:14:25Z Lukasz 2 uploaded a new version of &quot;[[File:AbstractBook2012.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 211 1431 2013-06-14T08:39:16Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 10 1442 1037 2013-06-24T17:22:48Z Lukasz 2 /* General */ wikitext text/x-wiki == General == [[Media:ScienceAlerts-general.pdf|Presentation in PDF]] describing the aims, design and methods of the entire Science Alerting system (from December 2009, not completely up-to-date). [[Media:AroundGaiaPoster2011.pdf | Poster]] on Gaia Alerts presented at the IAU Symposium #285 in Oxford in September 2011. [[Media:GaiaAlertsPosterIAUS298.pdf | Poster]] on Gaia Alerts presented at the IAU Symposium #298 in Chine in May 2013. Presentation of Gaia and Gaia Alerts with Prezi. <html> <div class="prezi-player"><style type="text/css" media="screen">.prezi-player { width: 550px; } .prezi-player-links { text-align: center; }</style><object id="prezi__3ghuqjeiq6k" name="prezi__3ghuqjeiq6k" classid="clsid:D27CDB6E-AE6D-11cf-96B8-444553540000" width="550" height="400"><param name="movie" value="http://prezi.com/bin/preziloader.swf"/><param name="allowfullscreen" value="true"/><param name="allowscriptaccess" value="always"/><param name="bgcolor" value="#ffffff"/><param name="flashvars" value="prezi_id=_3ghuqjeiq6k&amp;lock_to_path=0&amp;color=ffffff&amp;autoplay=no&amp;autohide_ctrls=0"/><embed id="preziEmbed__3ghuqjeiq6k" name="preziEmbed__3ghuqjeiq6k" src="http://prezi.com/bin/preziloader.swf" type="application/x-shockwave-flash" allowfullscreen="true" allowscriptaccess="always" width="550" height="400" bgcolor="#ffffff" flashvars="prezi_id=_3ghuqjeiq6k&amp;lock_to_path=0&amp;color=ffffff&amp;autoplay=no&amp;autohide_ctrls=0"></embed></object><div class="prezi-player-links"><p><a title="" href="http://prezi.com/_3ghuqjeiq6k/around-gaia-alerts-in-30-questions/">Around Gaia (Alerts) in 30 questions</a> on <a href="http://prezi.com">Prezi</a></p></div></div> </html> ---- ---- == Detection == Detection will be conducted in almost entire range of available magnitudes from Gaia. Limiting magnitude for Gaia is equivalent of V=20mag, but for detection we will require signal above at least 19mag, to avoid spurious anomalies at high noise level. The saturation limit for Gaia is around 5 mag. * '''Detection system employs the following data:''' ** newly acquired G-flux observations, 8-9 measurements separated by 4.4s (per-CCD) ** historical G-flux observations ** mean BP and RP colours ** low-dispersion BP and RP spectrometry (raw,uncalibrated) ** morphology of the source ** source motion flags ** later in the mission: CU3, CU4, CU7 and CU8’s deliverables (information on motion, variability, astrophysical parameters) == Sampling properties of Gaia == [[File:scanning_law_gal.png|400px|right|thumb|Number of observations per source over entire mission.]] Detections will be strongly affected by sampling properties of the Gaia. These are induced by characteristic "scanning law" (see figure). Gaia will be equipped with 2 telescopes, therefore there will usually be two subsequent observations of an object, separated by 106 minutes. Next scan comes after 6h after the first (4.5h after the last observation), so there may be another set of two fields of view observations, unless the satellite precesses enough to move to another bit of the sky. Then, the same object may be observed after 40-70 days, depending on the location. Such cadence allows for detection and immediate confirmation of an anomaly using closely spaced observations, but after the sequence, the object is gone for a long time from Gaia's view. [[File:gog_sampling.png|200px|left|thumb|Sampling distribution over the whole sky from Gaia simulator]] On the Gaia focal plane there are 8 or 9 (depending on alignment of the source on the plane) separate CCDs. The source will be observed by each of them with 4.4 seconds integration time. This feature can be very helpful in rejecting spurious anomalies, like cosmic rays, etc. Also, it will provide closely spaced observations, useful in detecting very rapid changes in brightness. '''[http://www.ast.cam.ac.uk/~wyrzykow/GAIA/gaia_scanning_anim_gal.mp4 Here] you can download a movie (40MB) showing Gaia scanning law (in galactic coordinates) and how number of observations per star is growing over the entire sky.''' == Photometric precision == [[File:Photometric_precision.png|300px]] From [http://arxiv.org/abs/0907.4084 M. Varadi et al. 2009]. == Classification == At this stage all additional information from Gaia and later from other catalogues will be used for narrowing down the sample of interesting alerts. == Cross-matching with existing catalogues == [[List of catalogues to cross-match]] 9ee58aeee2ddc4e39dfed3c9f6c3e6cbe50feaee 6 212 1443 2013-06-24T17:23:44Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 8 3 1448 1342 2013-06-25T09:36:22Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 18c98e093f6c955a9d84b8c3393d7d2b58493a37 0 1 1450 1332 2013-06-25T09:38:03Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- <center> '''<Big>[[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]]</Big>''' </center> ---- <center> [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 5326cbe6f4845cacac9f08cfeb92012484e93c68 6 213 1452 2013-06-26T17:15:42Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 204 1453 1451 2013-06-26T17:16:36Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop was held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics included: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invited all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda - archive of presentations]] * [[workshop2013:registration|Participants]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore * Iain Steele ---- Workshop Photo [[File:photo2013.jpg|500px]] 384f08e3b7a2087074f719bc31b1b639dc8318f2 1454 1453 2013-06-26T17:16:50Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2013.jpg|right|300px]] '''The fourth Gaia Science Alerts workshop was held in [[Workshop2013:logistics | Paris on 19-21 June 2013]].''' The topics included: * Status of Gaia - year of the launch! * Prospects for Gaia alerts * Preparation for the alerts follow-up and verification * Follow-up strategies * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners We invited all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2013:rationale|Rationale]] * [[workshop2013:agenda|Agenda - archive of presentations]] * [[workshop2013:registration|Participants]] * [[workshop2013:logistics|Logistic information]] <!--* [[workshop2013:poster|Workshop's poster for download]] --> ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Michel Dennefeld * Simon Hodgkin * Gerry Gilmore * Iain Steele ---- Workshop Photo [[File:photo2013.jpg|500px]] f578851cdbf625ec4021a8a974450f7b69e55272 0 200 1455 1323 2013-07-03T10:47:42Z Lukasz 2 changed the url of the server wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * IMPORTANT! The following fields must be selected in sextractor ''default.param'' file: [MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000] * Upload the sextractor output catalogue (by default ''test.cat'') to the Cambridge Photomretric Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F "matchDist=2" -F EventID='ivo://110610' -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 77ffd4fd21421a9351bce69971a774956cdcb9db 1459 1455 2013-07-12T10:52:50Z Lukasz 2 /* Calibration of your photometric data */ wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * IMPORTANT! The following fields must be selected in sextractor ''default.param'' file: [MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000] * Upload the sextractor output catalogue (by default ''test.cat'') to the Cambridge Photomretric Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/ The allowed formats for the sextractor catalogs are plain ascii and FITS. Obviously those catalogs must contain RA, DEC and MAG columns. == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 610f8d595375692cd1faa84095d1bceaca1079b8 1460 1459 2013-07-12T15:06:45Z Lukasz 2 wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * IMPORTANT! The following fields must be selected in sextractor ''default.param'' file: [MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000] * Upload the sextractor output catalogue (by default ''test.cat'') to the Cambridge Photomretric Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required: # MAG_AUTO # MAGERR_AUTO # ALPHA_J2000 # DELTA_J2000 ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.0), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 52f71b7ea77900e0f3a29ab458af71c1292e5786 0 203 1456 1322 2013-07-11T10:05:45Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia=== * Contact person: Goran Damljanovic * Location: Serbia * 60cm reflector === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 4e470672250fc21fb59c666dba15c5c1cc4fc487 1457 1456 2013-07-11T10:08:10Z Lukasz 2 /* Test no 1 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia=== * Contact person: Goran Damljanovic * Location: Serbia * 60cm reflector === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 95c5048483204a6523d4ee600afa620ac934970b 1458 1457 2013-07-11T10:08:28Z Lukasz 2 /* =ASV Serbia */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic * Location: Serbia * 60cm reflector === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 54f12c44bce6d26aad82c072af737f80ea734866 0 50 1461 539 2013-07-16T15:59:13Z Lukasz 2 wikitext text/x-wiki Close binary systems with orbital periods from 0.05 to 230 days. One of the components of these systems is a hot dwarf star that suddenly, during a time interval from one to several dozen or several hundred days, increases its brightness by 7-19 mag in V, then returns gradually to its former brightness over several months, years, or decades. Cool components may be giants, subgiants, or dwarfs of K-M type (from GCVS). * there is observed roughly 10 classical novae per year in the Milky Way and about 40 in other galaxies * absolute magnitude <math>M_V = -8 mag</math> * spectra near maximum light resemble A-F absorption spectra of luminous stars at first * spectra at minimum light resemble spectra of Wolf-Rayet stars. * amplitude between 7 and 19 mag in V * quick rise of few days * slow decline, between few days and 100 days (fast: type A, slow: type B, very slow: type C) * 15 days after maximum its Mv = -5.5mag, independent on speed or class * small changes at minimum light may be present Exemplary observations of a very fast nova with 0.3m Meade telescope: [[http://uk.arxiv.org/abs/1003.5371 Munari and Dallaporta]]. '''Recurrent novae''': * are produced by a white dwarf star and a red giant circling about each other in a close orbit * recurrent every 10-100 years * smaller amplitude: 4-9 mag * M_V at minimum is about 0-1 mag * example: RS Oph - 3 outbursts between 1957 and 1991 (AAVSO), exhibits some small variation in the baseline in minimum * decline within few days ---- Short transient searches in the other galaxies revealed possible new sub-class of novae: [http://uk.arxiv.org/abs/1003.1720 Kasliwal et al. 2010]. They usually stay above the Gaia detection limit for not more than 10 days. ---- Interesting paper on classification and properties of novae: [[http://uk.arxiv.org/abs/1004.3698 Strope, Schaefer & Henden 2010]] 59ea789023e7b5b1e346bb0475c3e74348b35ddf 0 17 1462 1307 2013-07-16T16:18:37Z Lukasz 2 /* Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h 149379ef14d8cbe9f1bb259e1035f0f202e4d531 0 1 1463 1450 2013-07-17T10:01:31Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- '''We are now creating the substructure WGs concentrating on broad science goals. See [[Working groups]] for details.''' ---- <center> '''<Big>[[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]]</Big>''' </center> ---- <center> [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- aae68335a6004d8f3b1e5c85fb17981b2ebcbd90 1464 1463 2013-07-17T10:02:07Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Structure == <center> '''We are now creating the substructure WGs concentrating on broad science goals. See [[Working groups]] for details.''' </center> ---- == Workshops == <center> '''<Big>[[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]]</Big>''' </center> ---- <center> [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 1e979e9d46384c1a441eb4430824c10e58d9d95b 0 214 1465 2013-07-17T10:05:17Z Lukasz 2 Created page with "Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon.Clark Eran Ofek === GSAWG2: CVs and XRBs === Si..." wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon.Clark Eran Ofek === GSAWG2: CVs and XRBs === Simon.Clark === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz === GSAWG5: AGNs and TDEs === Paul O'Brien Norbert Schartel === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon.Clark 4a1c6211c32c855472922a39df4972f192c2868e 1466 1465 2013-07-17T10:07:42Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon Clark Eran Ofek === GSAWG2: CVs and XRBs === Simon Clark Peter Jonker === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz === GSAWG5: AGNs and TDEs === Paul O'Brien Norbert Schartel Peter Jonker === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon Clark Patrick Tisserand d9ad4fec5ca71d3974eb5f889da9e24f95286981 1467 1466 2013-07-17T10:08:01Z Lukasz 2 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon Clark Eran Ofek === GSAWG2: CVs and XRBs === Simon Clark Peter Jonker === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz === GSAWG5: AGNs and TDEs === Paul O'Brien Norbert Schartel Peter Jonker Helene Sol === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon Clark Patrick Tisserand 80f681cf9a16ae8feba71ebc4db4b36c36a2deb7 1468 1467 2013-07-18T08:23:35Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon Clark Eran Ofek === GSAWG2: CVs and XRBs === Simon Clark Peter Jonker Zbigniew Kolaczkowski === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === Paul O'Brien Norbert Schartel Peter Jonker Helene Sol === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon Clark Patrick Tisserand Zbigniew Kolaczkowski 4ceb1432b5503c408d54035bc91acece4ff2976c 1469 1468 2013-07-18T08:24:54Z Lukasz 2 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon Clark Eran Ofek === GSAWG2: CVs and XRBs === Simon Clark Peter Jonker Zbigniew Kolaczkowski === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === Paul O'Brien Norbert Schartel Peter Jonker Helene Sol Stefanie Komossa === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon Clark Patrick Tisserand Zbigniew Kolaczkowski 28440b5fa58530ba5550036bb46e2639f535e869 1470 1469 2013-07-18T08:25:09Z Lukasz 2 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === Simon Clark Eran Ofek === GSAWG2: CVs and XRBs === Simon Clark Peter Jonker Zbigniew Kolaczkowski === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon Clark Patrick Tisserand Zbigniew Kolaczkowski 54fdd5970f7bd75e214a42216fa92bd42cd91ef7 1471 1470 2013-07-18T08:25:17Z Lukasz 2 /* GSAWG1: Supernovae (Core collapse, 1a) */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek === GSAWG2: CVs and XRBs === Simon Clark Peter Jonker Zbigniew Kolaczkowski === GSAWG3: Microlensing === Eran Ofek Rachel Street === GSAWG4: Young Stars === Aleks Scholz Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa === GSAWG6: GRBs === Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === Simon Clark Patrick Tisserand Zbigniew Kolaczkowski 49cb9a1d6c1efe10eac348da5bceafea464c60f8 1472 1471 2013-07-18T08:25:32Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa === GSAWG6: GRBs === #Paul O'Brien === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski a0fe945cf60cb438e037e967f34c9926616b32fe 1474 1472 2013-07-18T09:26:57Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski d78d3dcb3164cc76666d277a315a1b78581da67e 1481 1474 2013-07-22T11:06:24Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski ba7f91bba188f643e903499864042d17fdffdcd6 1482 1481 2013-07-22T11:45:54Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski e899bc959d798d1755b4e0ed69014c2b5ad23dbe 1483 1482 2013-07-22T12:18:13Z Gsawgwikiadmin 1 /* GSAWG2: CVs and XRBs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich.Kolb #Richard Busuttil === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski e617908f0e5e1ee8c8071970b2f7f24c3a2bacad 1484 1483 2013-07-23T14:31:35Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski dc369dc6a76fef7090e43374f43c17e940e8ef6a 1485 1484 2013-07-23T14:37:35Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke 833621817611e1f475708a0886d1cca960978e30 1486 1485 2013-07-24T12:23:50Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke fef93c0df97e7eee23e22f205808b5dc1f27df2d 1487 1486 2013-07-24T12:33:49Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke === GSAWG3: Microlensing === #Eran Ofek #Rachel Street === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke cb0623d7baedbac19e1aea827caba3e3a97da3b6 1488 1487 2013-07-24T12:37:01Z Gsawgwikiadmin 1 /* GSAWG3: Microlensing */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke 6925739904b3dabdf8f273119b0609aa76c7c0f2 1493 1488 2013-07-24T15:27:14Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them: === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke b9c70046834a8a62553252336b0012852eeaa348 1494 1493 2013-07-24T15:34:50Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke 375d66908fd431640f596d5182540170678fba43 1495 1494 2013-07-24T15:46:34Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke 05cf7442a4b7d06141cdd12f0e9e3de8d2c80721 1496 1495 2013-07-25T08:57:51Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock 1cec2d7287e4ae4d7454afc9fbce9474e09a8f2e 1497 1496 2013-07-26T09:26:31Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski fe28cfa3659b0bf42d0d8fb3aa497773fd36a072 8 3 1473 1448 2013-07-18T08:29:32Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 5950f615672ba06c3f049606cf21a9d5acc200b4 0 18 1475 338 2013-07-19T14:14:19Z Aleks.scholz 32 wikitext text/x-wiki == Eruptive YSOs == Prototypes: FU Oris are an extreme subsample of eruptive classical T Tauri stars. Only one outburst observed, but lasts for decades. Only about a dozen FU Ori bursts observed. FU Ori itself (V1647 Ori) is illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. EX Lupis (EXors) have smaller, shorter, recurrent outbursts [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. Characteristics: * diverse zoo of lightcurves * many details unknown, unbiased sample required * rise time varies from months to years * amplitude range from <1 mag to 5 mag * outburst last from months to decades * extreme events like FU Ori are very rare * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * At maximum spectral types are in the range Ae(alpha) - Gpe(alpha) * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) References: * Hartmann & Kenyon 1996 review: http://adsabs.harvard.edu/abs/1996ARA%26A..34..207H * Scholz et al. systematic survey: http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1301.3152 9dada4d856d7fbf44a7ca276a6d3d2fd6f5e8803 1476 1475 2013-07-19T14:18:14Z Aleks.scholz 32 wikitext text/x-wiki == Eruptive YSOs == Prototypes: FU Oris are an extreme subsample of eruptive classical T Tauri stars. Only one outburst observed, but lasts for decades. Only about a dozen FU Ori bursts observed. V1647 Ori is illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. EX Lupis (EXors) have smaller, shorter, recurrent outbursts. [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. Characteristics: * diverse zoo of lightcurves, use of templates is risky * many details unknown, unbiased sample required * rise time varies from months to years * amplitude range from <1 mag to 5 mag * outburst last from months to decades, some are recurrent * extreme events like FU Ori are very rare * Spectra: F or G supergiants * Spectrum: red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math>; in blue consistent with an early B spectral type * At maximum spectral types are in the range Ae(alpha) - Gpe(alpha) * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) References: * Hartmann & Kenyon 1996 review: http://adsabs.harvard.edu/abs/1996ARA%26A..34..207H * Scholz et al. systematic survey: http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1301.3152 ecc62659e67caa55746a4d521fa6551b8007f4e0 1489 1476 2013-07-24T14:30:35Z Aleks.scholz 32 wikitext text/x-wiki == Eruptive YSOs == Prototypes: FU Oris are an extreme subsample of eruptive classical T Tauri stars. Only one outburst observed, but lasts for decades. Only about a dozen FU Ori bursts observed. V1647 Ori is illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. EX Lupis (EXors) have smaller, shorter, recurrent outbursts. [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. Characteristics: * diverse zoo of lightcurves, use of templates is risky * many details unknown, unbiased sample required * rise time varies from months to years * amplitude range from <1 mag to 5 mag (but 1mag cutoff is probably useful) * outburst last from months to decades, some are recurrent * extreme events like FU Ori are very rare * Spectra: F or G supergiants, red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math> * At maximum spectral types are in the range Ae(alpha) - Gpe(alpha) * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) Trigger is necessary, because immediate follow-up (on timescales of weeks) needed to study the impact of such accretion bursts on the properties of the dust and gas in the disks. Also, high cadence monitoring immediately after the event is useful for modeling the source. References: * Hartmann & Kenyon 1996 review: http://adsabs.harvard.edu/abs/1996ARA%26A..34..207H * Scholz et al. 2013 systematic survey: http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1301.3152 * Clarke et al. 2005 with example lightcurves (Fig. 1): http://adsabs.harvard.edu/abs/2005MNRAS.361..942C 0d1f5ab24698352d40d814bb35ff88ed964eb862 1492 1489 2013-07-24T15:09:23Z Aleks.scholz 32 wikitext text/x-wiki == Eruptive YSOs == Prototypes: FU Oris are an extreme subsample of eruptive classical T Tauri stars. Only one outburst observed, but lasts for decades. Only about a dozen FU Ori bursts observed. V1647 Ori is illuminating a McNeil's nebula in the vicinity of NGC 2068 star-forming region. [[File:FUOri.png]] Plot from [http://www.ta3.sk/caosp/Eedition/FullTexts/vol36no3/pp149-157.pdf D.Chochol et al. 2006]. EX Lupis (EXors) have smaller, shorter, recurrent outbursts. [[File:ExLupi.png|right|400px|thumb|EX Lupi photometry from the ASAS project.]] OO Ser was discovered in 1994 and is similar to FUors and EXors, but is so deeply embedded, that at its brightest was not visible in J band ([http://ukads.nottingham.ac.uk/abs/1996ApJ...468..861H Hodapp et al. 1996]). It was observed in infrared with ''Infrared Space Observatory'' and Spitzer ([http://arxiv.org/abs/0705.1231 Kospal et al. 2007]). It has different time scales than FUors and EXors, is rather a ''fast'' FUor (similar to V1647 Ori) with a time of rise of about 8 months. Characteristics: * diverse zoo of lightcurves, use of templates is risky * many details unknown, unbiased sample required * rise time varies from months to years * amplitude range from <1 mag to 5 mag (but 1mag cutoff is probably useful) * outburst last from months to decades, some are recurrent * extreme events like FU Ori are very rare * Spectra: F or G supergiants, red, heavily veiled continuum with strong emission of <math>H_{\alpha}</math> * At maximum spectral types are in the range Ae(alpha) - Gpe(alpha) * X-ray variability present * FU Ori and V1057 Cyg rise over 1 yr, whereas V1515 Cyg rise over 20 years * FU Ori and V1515 Cyg decline over 20-100 years, V1015 Cyg decays faster (10 yrs) Trigger is necessary, because immediate follow-up (on timescales of weeks) needed to study the impact of such accretion bursts on the properties of the dust and gas in the disks. Also, high cadence monitoring immediately after the event is useful for modeling the source. Identification: * >1mag rise in magnitude * red spectrum, any spectral type * J-K>1. IR excess, UV excess * IRAC3 [5.8mu] - IRAC4 [8.0mu] > 0.4 * WISE1 [3.5mu] - WISE4 [22mu] > 2.0 * WISE1 [3.5mu] - WISE2 [4.5mu] > 0.3 (weak criterion) * Halpha emission References: * Hartmann & Kenyon 1996 review: http://adsabs.harvard.edu/abs/1996ARA%26A..34..207H * Scholz et al. 2013 systematic survey: http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1301.3152 * Clarke et al. 2005 with example lightcurves (Fig. 1): http://adsabs.harvard.edu/abs/2005MNRAS.361..942C ce69cbaed327586a613dad6c68becf81d089ff82 0 8 1477 670 2013-07-19T14:20:19Z Aleks.scholz 32 wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:FUOri | Eruptive young stellar objects]] * [[Triggers:YSOecl | Eclipsing young stellar objects]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:Supernovae | Supernovae]] * [[Triggers:TTau | T Tauri type pre-main sequence stars]] * [[Triggers:XBs | X-ray binaries (XBs)]] * [[Triggers:Other | Other rare transients]] * [[Triggers:Theoretical | Exotic/theoretical events]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 0f256fcdfa9c538b8328791c6b5b1290aa1d7f38 0 88 1478 292 2013-07-19T14:21:02Z Aleks.scholz 32 wikitext text/x-wiki == T Tauri stars == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>) pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. Characteristics: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful d82a9a2d668553de6c37b60f93b1695cf9fa0619 1498 1478 2013-07-26T10:19:25Z Chris.davis 34 /* T Tauri stars */ wikitext text/x-wiki == T Tauri stars == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>) pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. Characteristics: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] 7275ae666c2ef4ee2e0ef76645acb8226545db8c 1501 1498 2013-07-26T10:21:52Z Chris.davis 34 /* T Tauri stars */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>) pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. Characteristics: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] 33faa0a1680068fa0bf0d853742b7286df2d3b6f 0 215 1479 2013-07-19T14:38:41Z Aleks.scholz 32 Created page with "== Eclipsing young stellar objects == Characteristics: * long-lasting eclipses by disk material * shapes can be irregular * timescales days to years * high amplitudes possible (..." wikitext text/x-wiki == Eclipsing young stellar objects == Characteristics: * long-lasting eclipses by disk material * shapes can be irregular * timescales days to years * high amplitudes possible (several mags) * very few known, every new detection would help Examples: * KH15D recurrent, but changing eclipses- see Herbst et al. 2012 http://adsabs.harvard.edu/abs/2010AJ....140.2025H * RW Aur singular event - http://figshare.com/articles/A_huge_eclipse_in_the_young_star_RW_Aur/92169 * YLW 16 A has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P 62b1d9a12932ffecabec20ec0ba58f85927fc050 1480 1479 2013-07-19T14:41:59Z Aleks.scholz 32 wikitext text/x-wiki == Eclipsing young stellar objects == Characteristics: * long-lasting eclipses by disk material * shapes can be irregular * timescales days to years * high amplitudes possible (several mags) * very few known, every new detection would help Examples: * KH15D: recurrent, but changing eclipses- see Herbst et al. 2012 http://adsabs.harvard.edu/abs/2010AJ....140.2025H * RW Aur: singular event - http://figshare.com/articles/A_huge_eclipse_in_the_young_star_RW_Aur/92169 * YLW 16 A: has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P 7414543236e6d105c2eaf79500f097c912530a0d 1490 1480 2013-07-24T14:32:11Z Aleks.scholz 32 wikitext text/x-wiki == Eclipsing young stellar objects == Characteristics: * long-lasting eclipses by disk material * shapes can be irregular * timescales days to years * high amplitudes possible (several mags), cutoff of 1mag is probably useful * very few known, every new detection would help Trigger is necessary to figure out the origin of the eclipse -- the eclipsing body could be a part of the disk, clumps, protoplanetary structures, etc. Examples: * KH15D: recurrent, but changing eclipses- see Herbst et al. 2012 http://adsabs.harvard.edu/abs/2010AJ....140.2025H * RW Aur: singular event - http://figshare.com/articles/A_huge_eclipse_in_the_young_star_RW_Aur/92169 * YLW 16 A: has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P 275dc86c9ab70ae03e5843d82e666562e9f31219 1491 1490 2013-07-24T15:08:22Z Aleks.scholz 32 wikitext text/x-wiki == Eclipsing young stellar objects == Characteristics: * long-lasting eclipses by disk material * shapes can be irregular * timescales days to years * high amplitudes possible (several mags), cutoff of 1mag is probably useful * very few known, every new detection would help Trigger is necessary to figure out the origin of the eclipse -- the eclipsing body could be a part of the disk, clumps, protoplanetary structures, etc. Identification: * >1mag drop off in magnitude * red spectrum, any spectral type * J-K>1. IR excess, UV excess * IRAC3 [5.8mu] - IRAC4 [8.0mu] > 0.4 * WISE1 [3.5mu] - WISE4 [22mu] > 2.0 * WISE1 [3.5mu] - WISE2 [4.5mu] > 0.3 (weak criterion) * Halpha emission Examples: * KH15D: recurrent, but changing eclipses- see Herbst et al. 2012 http://adsabs.harvard.edu/abs/2010AJ....140.2025H * RW Aur: singular event - http://figshare.com/articles/A_huge_eclipse_in_the_young_star_RW_Aur/92169 * YLW 16 A: has smaller eclipses- http://adsabs.harvard.edu/abs/2013A%26A...554A.110P 5146447dc03cccd215c32ad160f5b7037e6a30eb 6 216 1499 2013-07-26T10:19:47Z Chris.davis 34 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 217 1500 2013-07-26T10:20:25Z Chris.davis 34 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 88 1502 1501 2013-07-26T10:31:38Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>) pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and are often associated with Herbig-Haro jets. Characteristics: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. FU Ori Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] ab941cd81f24a74cad9dfdc474b9df307238a75c 1503 1502 2013-07-26T10:47:08Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger ( <math> ~10^5 </math> y). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] be9fa57028820a78b6ee1145ed45f3dfd8308e3a 1504 1503 2013-07-26T10:50:10Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger ( <math> < 10^5 </math> y). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] 1f01af63df4646841efbde1803c30eadf09cc2a0 1505 1504 2013-07-26T10:51:03Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (<math> <10^5 </math> y). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] b686bdef4a1557686e8e1bb915ead381c374a76b 1506 1505 2013-07-26T10:52:29Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> y), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (<math> <100,000 </math> y). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] ac1044a59d6f81c4fc34ce050f23d84e266e4687 1507 1506 2013-07-26T10:52:49Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|400px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|400px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] eadce701ab474de2354e9a85a870220cc5e0c576 1508 1507 2013-07-26T10:53:38Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|500px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|500px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] 180d5aacc57c4ecb130eeb7bfcd9853f1f3935cf 1509 1508 2013-07-26T10:54:15Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki == T Tauri stars and other young variables and transients == [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. Relevant characteristics of TTSs: * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] e3275dc2083fbf9b3dd977029730737040c8a98b 1510 1509 2013-07-26T13:02:20Z Chris.davis 34 /* T Tauri stars and other young variables and transients */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs: == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features: == * Strong Balmer emission lines * Lithium absorption * P Cygni profiles == FU-Ori and EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] be9514d9792fc9f5619069e6207479f9c086c60d 1511 1510 2013-07-26T13:14:52Z Chris.davis 34 /* Spectral features: */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs: == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features: == * Strong Balmer emission lines * Strong forbidden emission lines; [OI], [SII], [NII], etc. * Lithium absorption * P Cygni profiles == FU-Ori and EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] 7c660b76fcd0fbf4d163e2b6b6fa085ce74c3757 1512 1511 2013-07-26T13:45:23Z Chris.davis 34 /* FU-Ori and EX-Ori and other outbursts */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs: == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features: == * Strong Balmer emission lines * Strong forbidden emission lines; [OI], [SII], [NII], etc. * Lithium absorption * P Cygni profiles == FU-Ori and EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] [[File:TTSvsFUor-spec.jpeg|900px|center|thumb|A comparison of red spectra for FU Ori and DG Tau]] 8b66e817ee71b3876e615ee4e488e3ccc7f5754f 1514 1512 2013-07-26T13:47:53Z Chris.davis 34 /* Spectral features: */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs: == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features == * Strong Balmer emission lines * Strong forbidden emission lines; [OI], [SII], [NII], etc. * Lithium absorption * P Cygni profiles == FU-Ori and EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] [[File:TTSvsFUor-spec.jpeg|900px|center|thumb|A comparison of red spectra for FU Ori and DG Tau]] 1632eb20b26e08c66583a58e3552cfb8b78b233e 1515 1514 2013-07-26T13:48:09Z Chris.davis 34 /* Relevant characteristics of TTSs: */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features == * Strong Balmer emission lines * Strong forbidden emission lines; [OI], [SII], [NII], etc. * Lithium absorption * P Cygni profiles == FU-Ori and EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] [[File:TTSvsFUor-spec.jpeg|900px|center|thumb|A comparison of red spectra for FU Ori and DG Tau]] cfa4b1becba4c775a6276a1e8de640091aea65e1 1516 1515 2013-07-26T13:48:42Z Chris.davis 34 /* Spectral features */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features == * Strong Balmer emission lines * Strong forbidden emission lines; [OI], [SII], [NII], etc. * Lithium absorption * P Cygni profiles (due to outflowing gas); inverse P Cygni in some cases == FU-Ori and EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] [[File:TTSvsFUor-spec.jpeg|900px|center|thumb|A comparison of red spectra for FU Ori and DG Tau]] fa2cf2e9d24e5872672845655db81cbd41ba6552 1517 1516 2013-07-26T15:10:05Z Chris.davis 34 /* FU-Ori and EX-Ori and other outbursts */ wikitext text/x-wiki = T Tauri stars and other young variables and transients = [[File:figure_ttau_mag.png|400px|right|thumb|T Cha - example of TTau star from the ASAS data]] T Tauri type stars (TTSs) are very young (<math> <10^7 </math> yr), low mass (<math> <3 M^{}_\odot </math>), pre-main sequence objects [http://adsabs.harvard.edu/abs/1989A%26ARv...1..291A Appenzeller & Mundt 1989]. They are optically visible (spectral type F,G,K,M) and their spectral energy distributions possess a modest excess in the near- and mid-IR, although the slope of their SED in the IR is still negative. Classical TTSs (Class II Young Stellar Objects) exhibit strong forbidden emission lines from ionised oxygen, sulphure, iron, etc., and they are often associated with Herbig-Haro jets; weak-lined TTSs (Class III YSOs) are essentially line-free. Class I YSOs possess a very strong IR excess (flat or positive spectral indices), are embedded, and are brighter in the near- and mid-IR bands. There is some statistical evidence that Class I YSOs - protostars - are the progenitors of TTSs; they are typically less abundant than Class II YSOs, are more likely to coincide with dark clouds and molecular cores, and may be much younger (< 100,000 yr). T Tauri stars are known to vary on periods of days, weeks, and months. Causes include episodic accretion events, warped disk occultations, the transit of dark spots in the photosphere. == Relevant characteristics of TTSs == * irregular and quasi-periodic variations * high amplitude (up to 5 mag) * may have a phase of quiescence (see figure) * absolute magnitude range: M_V=? to ? mag * typically do not require a trigger, but watch list of T Tauris would be useful == Spectral features == * Strong Balmer emission lines * Strong forbidden emission lines; [OI], [SII], [NII], etc. * Lithium absorption * P Cygni profiles (due to outflowing gas); inverse P Cygni in some cases == FU-Ori, EX-Ori and other outbursts == Some young pre-main-sequence stars have exhibited quite drastic episodic variations. 1-3 mag eruptions have been observed in several objects (e.g. EX Lup, DR Tau), while more spectacular eruptions corresponding to a brightening of 3-6 mag have been measured in FU Orionis type variables (FU-ors). A dozen young stars are now characterised as FUors. Most have been observed to rise 3-5 mag in brightness in less than one year; V1515 Cyg is the only known example to require a decade to rise to visual maximum. Note, however, that the historical light curves for many systems are poorly documented. Below are sample optical spectra of classical T Tauri stars and two FU-ori type eruptive variables. [[File:FUori-spectra.jpeg|450px|left|thumb|FRODOspec data from the Liverpool Telescope ]] [[File:CTTS-spectra.jpeg|450px|right|thumb|FRODOspec data of DG Tau (red), CW Tau (blue) and HL Tau (green) ]] [[File:TTSvsFUor-spec.jpeg|900px|center|thumb|A comparison of red spectra for FU Ori and DG Tau]] d3b6f4c82a69c96519053a5c9987382cf4bb747a 6 218 1513 2013-07-26T13:45:36Z Chris.davis 34 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 8 1518 1477 2013-07-26T15:14:13Z Chris.davis 34 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:FUOri | Eruptive young stellar objects]] * [[Triggers:YSOecl | Eclipsing young stellar objects]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:Supernovae | Supernovae]] * [[Triggers:TTau | T Tauri stars and other Young variables]] ** [[Triggers:FUOri | Eruptive young stellar objects]] ** [[Triggers:YSOecl | Eclipsing young stellar objects]] * [[Triggers:XBs | X-ray binaries (XBs)]] * [[Triggers:Other | Other rare transients]] * [[Triggers:Theoretical | Exotic/theoretical events]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 3fbb3831ce19985dbe2fa0f55ed23db696ede943 1519 1518 2013-07-26T15:14:36Z Chris.davis 34 /* Possible triggers for Science Alerts */ wikitext text/x-wiki ''' Please expand this section with your favourite types of possible alerts. The most useful information would be the number statistics, amplitude and timescale, example light curve, spectrum and the reasoning for an rapid alert.''' ===Possible triggers for Science Alerts=== * [[Triggers:Asteroids | Asteroids]] * [[Triggers:Be | Be-type stars]] * [[Triggers:CVs | Cataclysmic Variables (CVs)]] * [[Triggers:CNe | Classical novae]] * [[Triggers:DNe | Dwarf novae]] * [[Triggers:GRBs | Gamma Ray Bursts Optical Counterparts]] * [[Triggers:LensedSNe | Gravitationally lensed supernovae]] * [[Triggers:LBVs | Luminous Blue Variables]] * [[Triggers:Flares | M-dwarf flares]] * [[Triggers:Microlensing | Microlensing events]] * [[Triggers:RCrB | R Coronae Borealis type variables (dimming objects)]] * [[Triggers:Supernovae | Supernovae]] * [[Triggers:TTau | T Tauri stars and other Young variables]] ** [[Triggers:FUOri | Eruptive young stellar objects]] ** [[Triggers:YSOecl | Eclipsing young stellar objects]] * [[Triggers:XBs | X-ray binaries (XBs)]] * [[Triggers:Other | Other rare transients]] * [[Triggers:Theoretical | Exotic/theoretical events]] == Table of transients == This table is based on [http://arxiv.org/abs/0906.5355 Rau et al. 2009] on Palomar Transient Factory (PTF). MR is an absolute magnitude in R, tau is time of a decline by 2 mag. Note, these are not all the types of transites Gaia will detect. {| border="1" cellspacing="0" cellpadding="5" align="center" ! Class ! MR ! tau ! Universal rate ! Gaia rate |- | Dwarf Novae | 9..4 | 3..20 | <math>3\times10^{-5} \textrm{pc}^{-3} \textrm{yr}^{-1}</math> | |- |Classical Novae | -5..-10 |2..100 |<math>2\times10^{-10} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Luminous Red Novae | -10..-14 |20..60 |<math>1.5\times10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Fallback SNe | -4..-21 |0.5..2 |<math>10^{-13} \textrm{yr}^{-1}\textrm{L}_{\odot,K}^{-1}</math> | |- |Macronovae | -13..-15 |0.3..3 |<math>10^{-4..-8} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SN .Ia | -15..-17 |2..5 |<math>(4..10)\times 10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |SNe Ia | -17..-19.5 |30..70 |<math>3\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Tidal disruption flares | -15..-19 |30..350 |<math>10^{-6} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Core-collapse SNe | -14..-21 |20..300 |<math>5\times 10^{-5} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Luminous SNe | -19..-23 |50..400 |<math>10^{-7} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (SGRB) | -14..-18 |5..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |Orphan afterglows (LGRB) | -22..-26 |2..15 |<math>3\times 10^{-7..-9} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |On-axis LGRB afterglows | ..-37 |1..15 |<math>4\times 10^{-10} \textrm{Mpc}^{-3} \textrm{yr}^{-1}</math> | |- |} ---- == CMD of selected variables and transients == CMD paths of various types of variable stars, including Be stars, R CrB and V4334 Sgr. From [http://arxiv.org/abs/0907.4090 Spano et al. 2009] [[File:VariablesPathsCMDLMC.png|650px]] ---- == Time scales and amplitudes == [[File:Kulkarni-absmag-timescale.png|400px|left|thumb|Absolute magnitude vs timescale of novae, supernovae and some of new transients. From Kulkarni (2009).]] [[File:plot_transients_tau_ampl.png|400px]] [[File:plot_transients_trise_ampl.png|400px]] [[File:plot_transients_tdecline_ampl.png|400px]] [[File:plot_transients_trise_tdecline.png|400px]] 7f459f8fcb492e5eb46bb83a2d3a7a350f87b671 0 214 1520 1497 2013-07-29T08:55:07Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski b6e3247e5eb6932e5e331d4a28d6ad44f3490fc5 1521 1520 2013-07-29T13:46:35Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski 126ab83d0d7982329e65549208b1fb831e27f6f9 1522 1521 2013-07-29T13:48:24Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski e95a1bd854f0775d64e716aa7e7f70a54c2a23a4 1523 1522 2013-07-29T15:46:20Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley 9304ce1cddcc62bc51e95814a39e336b836602c0 1524 1523 2013-08-02T10:04:41Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley 83cdc090ae44dc8d7911b5d0d4cbeb8b4d7cdee4 1525 1524 2013-08-05T14:44:47Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Contreras, Carlos === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Stephen Potter === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley 1dc4c7bdfc593cc0c25bbee9ec2120eb106573a8 1527 1525 2013-08-16T21:25:13Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris J. Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Contreras, Carlos === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Stephen Potter === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley 6358235c3198457b7c6845fd569d04f4bb411d8a 1528 1527 2013-08-27T07:36:56Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Stephen Potter === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley 61a5a3094c2b9d87a6a0910eed4f939c4d009427 1529 1528 2013-09-02T12:00:02Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley 857168fc6a9a4ef6e37d8a017667366f1c6afd00 1530 1529 2013-09-02T14:17:56Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley ae6b9d3e8191cee213cdb64a4ac703e3083563c6 1531 1530 2013-09-09T10:27:05Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley === GSAWG8: Gaia Alerts Processing and Infrastructure === #Simon Hodgkin #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === 0c74128a91deb534978d82938b84555f7035fb68 1532 1531 2013-09-09T10:32:01Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley === GSAWG8: Gaia Alerts Processing and Infrastructure === *#Simon Hodgkin #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === 21aadaa5650c9b0c39707e827ba31096d6d20396 1533 1532 2013-09-09T10:32:39Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley === GSAWG8: Gaia Alerts Processing and Infrastructure === #*Simon Hodgkin #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === eda73dd7c120566edad6f21e3e338a4d316ed242 1534 1533 2013-09-09T10:33:21Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === 98427a218d33dddd7d1f6de48ca162b2a12b23d1 1535 1534 2013-09-09T15:17:10Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === 75568ff3e5a67fed57c5ea01025fb6d469f5ea6a 1536 1535 2013-09-09T16:00:54Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison #Dirk Froebrich === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === d6b6acd6a6fdb64873cfceff798b578375a296c1 1537 1536 2013-09-09T16:02:11Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wynn Evans #Francesca De Angeli #Giorga Busso === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === 75568ff3e5a67fed57c5ea01025fb6d469f5ea6a 1539 1537 2013-09-09T17:36:15Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === 28c1a574b2fdf157d4e8b96c82becdea02deac7c 1540 1539 2013-09-10T10:22:09Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === b058089cc04f75cf278067d632d7e6b6bb4e64c9 1541 1540 2013-09-10T10:54:56Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' 6cdaf19145d87e32eeaf7972ef3fdd8842cf7d5c 1543 1541 2013-09-12T15:15:00Z Sth 6 /* GSAWG1: Supernovae (Core collapse, 1a) */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' 34ff8621a275397d54113081db89d346cd7b5755 1544 1543 2013-09-12T15:15:15Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' 95d7eddf0c4d63feb55f331bf59ea249c6ef36ca 1547 1544 2013-09-13T09:49:09Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella #Stefanie Komossa === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' 4bbf90290511963194c8fd8f3d53eebf1d5ffb2a 1548 1547 2013-09-13T09:49:31Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella #Stefanie Komossa === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' 8ae2cb7d72feacb47be1c8721fab15e57c1494f2 1550 1548 2013-09-13T17:14:42Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt #Danny Steeghs === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella #Stefanie Komossa #Danny Steeghs === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' b492b3e08452e06781b00b5e6203c8af76dcec09 1551 1550 2013-09-13T18:47:21Z Andreja.gomboc 19 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt #Danny Steeghs === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch #Andreja Gomboc #Jure Japelj === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc 60ddad32a908c94f15da44a9aae47160864dc98f 6 181 1526 1324 2013-08-05T14:45:59Z Gsawgwikiadmin 1 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot;: launch 20.Nov wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1542 1526 2013-09-11T15:45:28Z Gsawgwikiadmin 1 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2 219 1538 2013-09-09T17:35:35Z Sth 6 Created page with "This is Simon Hodgkin" wikitext text/x-wiki This is Simon Hodgkin 78ba1bafe7cbffbe2118adcfaa860a4ac014a9ee 0 203 1545 1458 2013-09-13T08:49:13Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic * Location: Serbia * 60cm reflector ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 100cm and 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK bf6689b57b94cc0932e8f764732ef7ec143ea44e 1546 1545 2013-09-13T08:50:09Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic * Location: Serbia * 60cm reflector ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 100cm and 60cm ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 9ab488f5a58338cb3076d4d85b0cdfe6c8d2c422 1549 1546 2013-09-13T10:58:53Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic * Location: Serbia * 60cm reflector ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 361f11d75f401c109471b0fd11ab69f99c6011ec 0 214 1552 1551 2013-09-13T18:49:15Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt #Danny Steeghs === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch #Andreja Gomboc #Jure Japelj === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc 429dd1bc5915b9c886465202406129606e607d69 1553 1552 2013-09-13T18:52:42Z Sth 6 /* GSAWG6: GRBs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan #Sjoert van Velzen #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski #Morgan Fraser #Lina Tomasella === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair #Chris Copperwheat #Peter Wheatley #Stephen Potter #Elme Breedt #Danny Steeghs === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan #'''Sjoert van Velzen''' #Stephen Potter #Elme Breedt #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan #David Alexander Kann #Matthew Schurch #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc e84110f8fe100142a6d8a8414a92776cdc95c0ee 1554 1553 2013-09-13T19:14:32Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] 63299c4ed278af4d0f61c204a027470d4ef70764 1555 1554 2013-09-13T19:15:19Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] 6a3670fd944352361577a0769836df7171b3df94 1556 1555 2013-09-13T19:20:16Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] 6903b3f06382c63704a05668f2eedbe839aeedc6 1557 1556 2013-09-13T19:23:08Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] 1ad6340b5b8fd4f928660f4ab59271cffeb6a282 1558 1557 2013-09-13T20:40:13Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] 0c285a6747fb3fac48939171ad03447a597a1072 1559 1558 2013-09-13T21:22:26Z Sth 6 /* GSAWG8: Gaia Alerts Processing and Infrastructure */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] faf43e120895a59d0750ce9e447e367b5455787e 1560 1559 2013-09-13T23:08:08Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] 52e6e1ed918c95794414cea1aa29c9249f8a5aed 1561 1560 2013-09-13T23:11:34Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] 4291c298acd5f3a1fe810837f10c3cfec216ccc7 1562 1561 2013-09-13T23:13:31Z Sth 6 /* GSAWG10: Photometric Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley 47e5663631d90b8b246533df03a27736b9514df8 1563 1562 2013-09-13T23:35:02Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Elme Breedt [O] #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley ee82587a3b4a2f4ba4658400822217e3be500f8c 1564 1563 2013-09-13T23:47:42Z Sth 6 /* GSAWG2: CVs and XRBs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley 82b1edd72f44a70feadf426cc229d5293a942459 1565 1564 2013-09-13T23:53:02Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley 272a72c4ad380da0dde951592a1dec7da79c3362 1566 1565 2013-09-13T23:56:27Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina da8cf1524c3aa1090423d1b248cc170b1717cfb3 1567 1566 2013-09-14T00:13:05Z Sth 6 /* GSAWG2: CVs and XRBs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina 4020306e024e8e06b81eed3b1c5853ccaca478e1 1568 1567 2013-09-14T14:49:25Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina 39b79eb160b1a22b278a45e77f7b2a0a2677d679 1569 1568 2013-09-14T14:58:22Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina fb44b92b651bbca784fa8cec307dfdc0271191e0 1570 1569 2013-09-14T15:08:44Z Sth 6 /* GSAWG8: Gaia Alerts Processing and Infrastructure */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina 20380e73c29559cb88f9624a5e404dd8b3e212ca 1571 1570 2013-09-14T15:11:29Z Sth 6 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina 9d841a076914ec0f5673e00d0a523ec19ad8eee0 1572 1571 2013-09-14T15:11:53Z Sth 6 /* GSAWG10: Photometric Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal 8f8cea7220605537a2db2f5a703d47f848982c51 1573 1572 2013-09-14T15:13:28Z Sth 6 /* GSAWG8: Gaia Alerts Processing and Infrastructure */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal c720bcfae0d595244dfaf58388d99e5bf89b1331 1574 1573 2013-09-15T09:44:55Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #Simon Hodgkin (PI INT spectroscopy programme) [O] #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal d50a996483e87d0f454f15b651cd11a37e2e3fd9 1575 1574 2013-09-15T09:45:20Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal dbdcf064130f02d60cf7e78763aff9e83a8f01de 1577 1575 2013-09-15T15:06:38Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal b224d56fd18cec67a1acc24d5d78221dacf338ec 1579 1577 2013-09-15T22:39:32Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal bbb6a1d41c061b83b000ddae885d6e86f8548321 1580 1579 2013-09-15T22:39:46Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal 9bd475ef9f8f317737f8b7aecafb4e3349bd1a26 1581 1580 2013-09-15T23:06:20Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal c938631fa549bd1994f730abeff62e0a72f3e8e9 1582 1581 2013-09-16T13:58:52Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley #Cecilia Farina #Ashish Mahabal b76fedb0e53dfac61bbc7a0e6c238796eaf6e159 1583 1582 2013-09-16T15:04:39Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] a0b78d8025cde1bb3a87f32f636d6d65ee8e60ed 1584 1583 2013-09-16T15:05:16Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] 847e3a90ca93bc329e18de3330532fc6ca60e81d 1585 1584 2013-09-16T16:20:04Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky 85d000ece74a40b6a299c5e23cd59c503a003e4b 1586 1585 2013-09-17T10:11:21Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky 343fea6056edbb50f70ddbee2fa7cb97b5925223 1587 1586 2013-09-19T12:03:27Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #Lukasz Wyrzykowski #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James a9349d4f5e7d29aaa9eb5aee89b65e4bfb35df37 1588 1587 2013-09-19T12:11:44Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin (PI INT spectroscopy programme) [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James f7beb47099b60cb517f8729b0b1466f1c4cd3e5f 6 220 1576 2013-09-15T10:02:11Z Sth 6 Proposal submitted to INT for Semester 2014A wikitext text/x-wiki Proposal submitted to INT for Semester 2014A a6b1a17a7a81f1c54868ee018782c68cf131f0e5 6 221 1578 2013-09-15T22:38:34Z Sth 6 WHT Proposal wikitext text/x-wiki WHT Proposal 9be3cc292b11267d04e17d25214419040e3e0026 0 203 1589 1549 2013-09-29T10:14:27Z Lukasz 2 /* ASV Serbia */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Tests: July 2013, automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 43793adbb8b848acd99f689dae81791dd7be1337 1590 1589 2013-09-29T10:15:01Z Lukasz 2 /* pt5m */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Tests: July 2013, automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Tests: July 2013, automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 4bc2d3034b6b51860dae1e24e175f6830a94a0fd 1591 1590 2013-09-29T10:15:13Z Lukasz 2 /* pt5m */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Tests: July 2013, automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 6b28eb8055b20fcc3fd678cc1599391f368aaec4 1592 1591 2013-09-29T10:15:23Z Lukasz 2 /* ASV Serbia */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK eb59dfbe16f8cc64a3f85d593e2599ecd6b9d2c0 1593 1592 2013-09-29T10:15:55Z Lukasz 2 /* Tubitak Turkey */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 76c4165d03e248a63814547844004f1e6081b31a 1594 1593 2013-09-29T10:16:35Z Lukasz 2 /* Vienna */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 71326d5b7955e9b7b798470d9c9012ff8e14e9c4 1595 1594 2013-09-29T10:16:51Z Lukasz 2 /* PIRATE */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''tests: ''' 2011 ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 9746e4480b9f27dccc1aa2ab98226843039e4e6f 1596 1595 2013-09-29T10:17:17Z Lukasz 2 /* Loiano */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 8a918bfbb04d632b57dfc1cd60334f28b189c632 1597 1596 2013-09-29T10:17:47Z Lukasz 2 /* Bialkow/Wroclaw Poland */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before September 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 610ce3ca8ed50dfd486d645746aa103538e5f721 1598 1597 2013-09-29T10:18:10Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Partners in test== === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK fdc8016a908ecc05429bec7462666d80e40b5915 1599 1598 2013-09-29T10:19:47Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 024f61f81de77234aaf6006b0f5069a09b3d0b17 1600 1599 2013-09-29T11:56:45Z Lukasz 2 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia [[File:ASASSN-13dd-RTT150-r.png]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 1189a9fa06dc336c12db9b88457039d5974f7fa6 6 222 1601 2013-09-29T11:57:14Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 203 1602 1600 2013-09-29T11:57:34Z Lukasz 2 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia [[File:ASASSN-13dd-RTT150-r.png:right:200pix]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK b4044a8afaff518e365d455ec12612baaf1dcf54 1603 1602 2013-09-29T11:57:45Z Lukasz 2 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia [[File:ASASSN-13dd-RTT150-r.png|right|200pix]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 97059ada8b90b5689bf24c4a6400195f206f79db 1604 1603 2013-09-29T11:58:17Z Lukasz 2 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia [[File:ASASSN-13dd-RTT150-r.png|right|200px ASASSN-13dd captured by RTT150 on 29.Sep 2013]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK b48934cfd4416317a67b80be4424164601000d55 1605 1604 2013-09-29T11:58:29Z Lukasz 2 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia [[File:ASASSN-13dd-RTT150-r.png|right|200px|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK b7ce275e40ff8f48df1d57869d6ac55596c2da9f 1606 1605 2013-09-29T12:00:12Z Lukasz 2 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK f404f7884c787873fd3a42bc30fc6fb7f5676fb1 1627 1606 2013-10-11T10:55:27Z Gsawgwikiadmin 1 /* Test no 3 */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 913c3747d8c2dd65a2dccac69e424b6d625bfec8 1628 1627 2013-10-11T10:55:45Z Gsawgwikiadmin 1 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) # perform at least 5 (TBC) tests before December 2013. (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK d02eb7f66470351a8b1d8ab46a60723c391397c5 0 214 1607 1588 2013-09-30T15:39:54Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James 0539dc628851908fbefb21f27a04cebde61e3550 1608 1607 2013-09-30T15:41:10Z Sth 6 /* GSAWG2: CVs and XRBs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James 791b1c25918fe4da0ac6cb5663f632d159dc9b5f 1609 1608 2013-09-30T16:45:59Z Sth 6 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James 9358c82aa659b87360e658475b885387ed35c44f 1610 1609 2013-09-30T16:47:32Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James 997a7230b460fee0438cee54a3cf8ac42516c4eb 1611 1610 2013-09-30T16:49:48Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov deab8f651782156af3dfeebec294136dcbc23f59 1612 1611 2013-09-30T16:50:54Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 23f99930545d14ccf653eb134b51b0458b7d78f9 1613 1612 2013-09-30T16:55:38Z Sth 6 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 8e8ac57ffc8f092e8104bf065506e83e82a9c1e5 1614 1613 2013-10-01T07:30:29Z Sth 6 /* GSAWG1: Supernovae (Core collapse, 1a) */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 93031378b0235acec731a149b9a256cc67356c34 1615 1614 2013-10-01T07:30:55Z Sth 6 /* GSAWG2: CVs and XRBs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov e375a0cff54222731234ee81b71fd801f4191d69 1616 1615 2013-10-01T07:32:10Z Sth 6 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 3682d18bb44c6121326126b6ac5e0736fd502d60 1618 1616 2013-10-01T09:46:07Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Nic Walton [O] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 541243324820b318bb020d5ba7381016ab6ee42a 1619 1618 2013-10-03T02:52:08Z Nic.walton 35 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 1778df4e5d4cd69d235738bfc927e4dc86dc7d42 1621 1619 2013-10-07T09:21:24Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [ http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 2d4b91f40cf61bfd5b9b4b43113c33e4f35e107d 1622 1621 2013-10-07T09:21:45Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 534d697d2db2a2585263997878a08018641989a2 1624 1622 2013-10-07T09:25:10Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 582e844eda42efb635134ddebedbbed045ed5eab 1625 1624 2013-10-07T09:25:27Z Sth 6 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov 563c74d89cc9f41e0271ed6cc178ac1704b87e85 1626 1625 2013-10-10T13:57:27Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya 70d00d20594a95462687255bd23b1a97edad35e2 1629 1626 2013-10-14T14:52:20Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto bbf40ea88d29aa886d82810b4a94974f45f3c56d 1634 1629 2013-11-07T15:56:56Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto e367558fa98c210e6cc0259661b837cdb6e60f60 1635 1634 2013-11-22T08:52:09Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto 6732a01e4a63a175744bb9a7da8884759b0535d0 1637 1635 2013-12-09T13:51:03Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto 3616aa9b263c83c182b8a63ad582ddc02b72487d 1639 1637 2013-12-19T09:29:56Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti *Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto 6078facd2afe62dac1089e79b58380a10b374ad1 1640 1639 2013-12-19T09:30:09Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto f9d0c5923484f39aaad3fa861b17d28f67149697 1641 1640 2013-12-19T09:31:13Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #Chris Davis [O] #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto ae6b8bf3da12f4fb113cd607525252ca81331a47 1642 1641 2013-12-19T09:31:35Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto be6ec90e8483f063dc97772e929ecc7331b7e7be 1643 1642 2014-01-15T11:05:07Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla bc536b498b84298c7a59673778fbba3927c2c945 1644 1643 2014-02-20T09:05:40Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic bd9093093e8f0f81aa55fe29d5d804c3d1c9d5a6 1645 1644 2014-02-20T14:39:25Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet a2b074665fae74492d2045100898825fdf8c71eb 1646 1645 2014-02-23T20:49:05Z Nic.walton 35 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 294188238eea1c4c8726c905dfd57d727a70587a 1647 1646 2014-03-06T21:51:25Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars === #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 193fb247ad61d405069c27226453507bc698f4a6 1648 1647 2014-03-07T17:39:03Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === GSAWG4: Young Stars [http://wiki.astro.ljmu.ac.uk/YoungTransients/ | WG Wiki (password protected)]=== #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 2e8b496cb7e6dc3289083d536e24e558fcce5de3 1649 1648 2014-03-07T17:41:02Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === '''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet f84a3b202a6a1279a651422544ecab97b6629149 1650 1649 2014-03-07T17:41:15Z Lukasz 2 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet ddc7ede5cc720f1e89b4e02651e3e473a90dc768 1651 1650 2014-03-10T11:29:51Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet f0cc09805b891f00312a06cdcecd56e24f7a76a0 6 223 1617 2013-10-01T09:44:43Z Sth 6 ESO proposal for NTT+EFOSC2 follow-up : 093.D-0856 wikitext text/x-wiki ESO proposal for NTT+EFOSC2 follow-up : 093.D-0856 e0a1d287928185d63c85dfae8fc00aca8e327f97 6 224 1620 2013-10-07T09:19:45Z Sth 6 PATT: Liverpool Telescope follow-up proposal Semester 14A wikitext text/x-wiki PATT: Liverpool Telescope follow-up proposal Semester 14A 450941ec6d6bd304ec5750a0860e29765a2c30eb 6 225 1623 2013-10-07T09:24:02Z Sth 6 JMU TAC version of LT follow-up proposal wikitext text/x-wiki JMU TAC version of LT follow-up proposal a076b18c18cc99bee9489d3277803d5b326f7fe2 0 200 1630 1460 2013-10-23T07:41:23Z Lukasz 2 wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your '''default.sex''' configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in '''default.params''': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in '''default.sex''' as: CATALOG_TYPE ASCII_HEAD ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.0), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 922248b910eabeb7b36756b3c98d3d125aa07064 1631 1630 2013-10-23T07:42:11Z Lukasz 2 wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.0), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org c18c6168c8ed70551738b8f9afcfa4d419567856 1632 1631 2013-10-23T07:42:37Z Lukasz 2 wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org cf82b5189adb0fe889f0b2abfa37962e6033618a 1636 1632 2013-12-06T08:47:29Z Lukasz 2 /* Data format */ wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on) ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org f2e1cdcde7430f07b556786a6731e994ff1d27d5 6 181 1633 1542 2013-11-01T00:20:15Z Gsawgwikiadmin 1 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot;: Launch 20 Dec. wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1638 1633 2013-12-12T17:20:19Z Lukasz 2 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot;: 19 Dec launch wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 214 1652 1651 2014-03-11T09:08:21Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet f0405f2a100d4b4ddaa0f8c22cdda7810cdce5b4 1653 1652 2014-03-11T09:09:05Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet b3b9af0079a0ea1acb88c556137a44c6eef506d6 1654 1653 2014-03-12T10:52:22Z Chris.davis 34 /* GSAWG4: Young Stars */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet ba19c552e107d1136f217827621ad3a8f6708ab3 1678 1654 2014-03-15T19:13:29Z Sth 6 /* GSAWG1: Supernovae (Core collapse, 1a) */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 68c169c8ed37c919621c2d0fb04b0081d624865c 1679 1678 2014-03-15T19:26:42Z Sth 6 /* GSAWG1: Supernovae (Core collapse, 1a) */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 642dcbb3513ce256a192064ce7424fe04116c8c3 1680 1679 2014-03-15T19:29:55Z Sth 6 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet b13d594b1a5728709b05ab68b1eacf62487705b0 1681 1680 2014-03-15T19:30:50Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 5b3636ddaf7ce1fde639830df0d127b05653fead 1682 1681 2014-03-15T19:32:07Z Sth 6 /* GSAWG9: Spectroscopic Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 8c2702e2a0ff5de683f8ce84c648eb846ff62497 0 1 1655 1464 2014-03-12T12:44:52Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Structure == <center> '''We are now creating the substructure WGs concentrating on broad science goals. See [[Working groups]] for details.''' </center> ---- == Workshops == <center> '''<Big>[[Workshop2014:main|5th Gaia Science Alerts Workshop 2014, Warsaw]]</Big>''' </center> ---- <center> [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- c1bb254e3b5b869630e779caf2449511ba6e601b 8 3 1656 1473 2014-03-12T12:50:07Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2014 **workshop2014:main|Main Workshop Page **workshop2014:rationale|Rationale **workshop2014:agenda|Program **workshop2014:registration|Participants and Registration **workshop2014:logistics|Logistics * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 0838b389d8f4bb5eedcc1d498587d903f59b37b2 0 226 1657 2014-03-12T13:00:43Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2014.jpg|right|300px]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The ..." wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * Follow-up strategies * Machine learning approaches to the classification of transients * Current/planned multi-wavelength transient surveys * Reports from tests on transient follow-up * Presentation of new partners * Building training sets * Supernovae, Microlensing, Novae, GRBs, TDEs, CVs * Verification phase We invite all researchers and observers interested in getting ready for and taking part in the exciting era of Gaia transients observations. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Szymon Kozlowski LOC: * 689d789ecafdd86d2f63f09667b07835f4ad855e 1658 1657 2014-03-12T13:02:45Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Szymon Kozlowski LOC: * c5f75e0de8f6bf59b8c296f945411ddfbb8773fb 1672 1658 2014-03-12T13:48:34Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Szymon Kozlowski LOC: * 12dbd98620736c40d450f7f7adc31a91a6c48185 1673 1672 2014-03-12T13:50:14Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Szymon Kozlowski LOC: * 8f1e2bd98fe8365f7663463454352bfe8b5877f4 1675 1673 2014-03-13T12:01:42Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organizing Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Szymon Kozlowski LOC: * Zuzanna Kostrzewa-Rutkowska * Alicja Rynkiewicz * Lukasz Wyrzykowski * Szymon Kozlowski c52778787f5d9cfcf6d93dbe04f547a97791580f 0 227 1659 2014-03-12T13:24:12Z Gsawgwikiadmin 1 Created page with "=Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, ..." wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:buw-foto.jpg]] 3ce9fefc1cd80aa155bd5fa8b18cf4d976cfc67d 1661 1659 2014-03-12T13:27:00Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:buw-foto.jpg]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. [[File:buw-sal.jpg | Main auditorium ]] On the 12 September the splinters will take place in two smaller rooms nearby. 74cd523986a4aa18b27b7cc47ce6a48c9cc6eb04 1663 1661 2014-03-12T13:27:58Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:buw-foto.jpg]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. [[File:buw-sal.jpg|250px| Main auditorium ]] On the 12 September the splinters will take place in two smaller rooms nearby. 14330d4c1333bfe45e76762a952a26a8521face7 1664 1663 2014-03-12T13:30:56Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:buw-foto.jpg]] The Library is located at ul. Dobra 56/66 and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). [[File:map.png]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. [[File:buw-sal.jpg|250px| Main auditorium ]] On the 12 September the splinters will take place in two smaller rooms nearby. 3d2438743c1e8d21e103efae53f7da4e642da9c7 1666 1664 2014-03-12T13:31:56Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:buw-foto.jpg|right]] The Library is located at ul. Dobra 56/66 and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). [[File:map.png|right]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. [[File:buw-sal.jpg|250px| Main auditorium ]] On the 12 September the splinters will take place in two smaller rooms nearby. 497913158399f2f4a3b0bc07c266d8bf97e90a92 1667 1666 2014-03-12T13:32:10Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:buw-foto.jpg|right]] The Library is located at ul. Dobra 56/66 and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). [[File:map.png|300px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. [[File:buw-sal.jpg|250px| Main auditorium ]] On the 12 September the splinters will take place in two smaller rooms nearby. 992af0c416d980434b06fd0bc5ce5ee053a4c6c1 1668 1667 2014-03-12T13:32:32Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at ul. Dobra 56/66 and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). [[File:map.png|300px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] On the 12 September the splinters will take place in two smaller rooms nearby. 822bcb0da4b6dd40312ceae9d2bebf8c1ceab3ca 1669 1668 2014-03-12T13:32:46Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at ul. Dobra 56/66 and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). [[File:map.png|300px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] c611d6cab8c6840411e1004ac7f738d35083dee9 1670 1669 2014-03-12T13:32:56Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at ul. Dobra 56/66 and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). [[File:map.png|500px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] de458a8d61125abef6d0201fb83843c2621e91f9 1671 1670 2014-03-12T13:42:54Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] d1765d22385b6a978f97f29e8dc43936e0d962d9 1674 1671 2014-03-12T14:47:23Z Gsawgwikiadmin 1 wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague (to Warszawa Gdanska) and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * SOFITEL * Harenda * Castle Inn e19a47bc4978099316a60c141516d7f0e1534786 1676 1674 2014-03-15T15:01:43Z Zuzanna 36 /* By Train */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 128 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * SOFITEL * Harenda * Castle Inn 0da1f7b2b68a1763993e47eead2c0f149bdd4b03 1677 1676 2014-03-15T16:19:40Z Zuzanna 36 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * SOFITEL * Harenda * Castle Inn fd4caaf8e8e3cc6fc35260285cf2d3c915dccbd3 1683 1677 2014-03-16T11:57:14Z Zuzanna 36 /* Accommodation */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] * [http://www.hotellogos.pl/en/ Logos] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] b6104ac43986a03df96eab5432f9813c234626a3 1685 1683 2014-03-24T01:11:52Z Lukasz 2 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] * [http://www.hotellogos.pl/en/ Logos] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 9925fd5b248e4e4f60e30621e0f41cb4556b80d5 6 228 1660 2014-03-12T13:24:25Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 229 1662 2014-03-12T13:27:09Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 230 1665 2014-03-12T13:31:06Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 86 1684 274 2014-03-21T00:23:06Z Lukasz 2 wikitext text/x-wiki List of catalogues to be used for cross-matching Gaia Science Alerts sources: * SDSS * 2MASS * NED * ASAS [http://www.astrouw.edu.pl/asas/] - long term photometry data in I and V. Whole sky (N+S), down to 14mag * OGLE [http://ogle.astrouw.edu.pl] - long term photometry data in I and V. Bulge and Magellanic Clouds only * INTEGRAL [http://arxiv.org/abs/0910.1704] - Gamma-ray sources, all sky, data available for download [http://integral.esac.esa.int/isda/] * WISE all sky infrared catalogue b8515451440e69c9c3626e9ad911f41dd19cb7ae 0 231 1686 2014-03-24T01:17:27Z Lukasz 2 Created page with "The preliminary outline of the workshop: * 9.Sep, Tuesday, workshop commences in the afternoon * 10.Sep, Wednesday, full day, workshop dinner in the evening * 11. Sep, Thursday,..." wikitext text/x-wiki The preliminary outline of the workshop: * 9.Sep, Tuesday, workshop commences in the afternoon * 10.Sep, Wednesday, full day, workshop dinner in the evening * 11. Sep, Thursday, full day * 12. Sep, Friday, splinter sessions, hands-on, workshop closes after lunch c4b77970008ded452d8b072622f5f735ea789bc7 0 232 1687 2014-03-24T19:29:33Z Lukasz 2 Created page with "== Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiascienc..." wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiasciencealertsworkshop2014@gmail.com'' ---- {{#form: action=<nowiki>http://www.ast.cam.ac.uk/~wyrzykow/cgi-bin/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Wednesday 10th''''' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 0e1986c18a5a776e221332a62aa55c616a2870bc 1688 1687 2014-03-24T20:49:34Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiasciencealertsworkshop2014@gmail.com'' ---- {{#form: action=<nowiki>http://www.astrouw.edu.pl/ּּ~wyrzykow/exec/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Wednesday 10th''''' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 64eed0c4e4bd2cedd93a421f0dbbeb502f3182ab 1689 1688 2014-03-24T20:51:39Z Lukasz 2 wikitext text/x-wiki == Registration form == '''If you have already send this form, please do not send it again!''' In order to amend you application or with other queries please email ''gaiasciencealertsworkshop2014@gmail.com'' ---- {{#form: action=<nowiki>http://www.astrouw.edu.pl/~wyrzykow/exec/mailer.cgi</nowiki> | method=post}} '''Contact details''' {| |- |Title (Mr/Mrs/Dr/Prof): | {{#input:type=textarea|name=dr|cols=5|style=width:auto|rows=1}} |- |Name: | {{#input:type=text|name=name}} |- |Affiliation: | {{#input:type=textarea|name=affiliation|cols=50|style=width:auto|rows=1}} |- |Work address: |{{#input:type=textarea|name=address|rows=3|cols=30|style=width:auto}} |- | Telephone: | {{#input:type=textarea|name=tel|value=don't forget your country code|cols=30|style=width:auto|rows=1}} |- |Email: |{{#input:type=textarea|name=email|rows=1|cols=20|style=width:auto}} |} {{#input:type=hidden|name=wabik}} ''Please give a short description of your current research and research interests, as well as a description of how you will contribute to and benefit from the workshop (<400 words)'' {{#input:type=textarea|name=research|rows=6|cols=100|style=width:auto}} ---- {| |- | '''My contribution to the Workshop:''' |{{#input:type=select|name=contribution| *Please select *talk *none}} |} {| |- | Title: | {{#input:type=textarea|name=title|rows=1|cols=100|style=width:auto}} |- | Brief abstract: | {{#input:type=textarea|name=abstract|rows=4|cols=100|style=width:auto}} |} ---- '''Social Dinner''' ''We plan to have a workshop's dinner on'' '''''Wednesday 10th''''' {| |- | I would like to participate in the dinner: | {{#input:type=select|name=dinner| *Please select *yes *no}} |} ---- '''Other''' {| |- | Special dietary requirements (e.g. vegetarian, vegan): | {{#input:type=text|name=diet|value=No special dietary requirements}} |} {| |- | Disabled access: | {{#input:type=text|name=disabled|value=No special disabled requirements}} |} ---- '''Funding''' Should you request any funding support, please email us directly with a justification and an estimate of the travel and accommodation costs. The support is available primarily for students and postdocs.''' ---- '''Now, make sure everything you entered is ok. If form is processed successfully you will receive a confirmation email.''' ---- {{#input:type=submit|value=Send}} {{#formend:}} 6bd720e0638f9e180c01e65cb5f70b184e339747 0 233 1690 2014-03-25T04:54:15Z Lukasz 2 Created page with "<big>'''The registration is now open!'''</big> Please fill the registration form [[Workshop2014:registrationform here]] by 31st July 2014. List of registered participants: #" wikitext text/x-wiki <big>'''The registration is now open!'''</big> Please fill the registration form [[Workshop2014:registrationform here]] by 31st July 2014. List of registered participants: # 21bb3d0aec09b0fa731e367bcd8a05a148942e5e 1691 1690 2014-03-25T04:54:28Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> Please fill the registration form [[Workshop2014:registrationform|here]] by 31st July 2014. List of registered participants: # ae369e47e626194793873b73db357b31be2970b0 1692 1691 2014-03-25T04:54:53Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form]] by '''31st July 2014'''. List of registered participants: # bf41fbc7ddcc62716f02ae72202c2320afef1442 1693 1692 2014-03-25T04:55:05Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. List of registered participants: # 561d522c52ece74dd2fcbaff9bdd5d778da50e19 1694 1693 2014-03-25T04:55:27Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. == List of registered participants: == # 6f6aa8058741767fbe1aebed813b79b90e1dcbbb 1695 1694 2014-03-25T04:55:37Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. === List of registered participants: === # 0053eff4349e0a9282a8476b696dc5f35ba00892 1696 1695 2014-03-25T04:55:44Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. ==== List of registered participants: ==== # 138b32208d3362ad0bdb3b3fdff379efdae6c8b6 1697 1696 2014-03-25T04:55:53Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. ===== List of registered participants: ===== # fafa3c205fda2ab39989b6e909502c70ee25fa8a 0 234 1698 2014-03-25T05:06:06Z Lukasz 2 Created page with "'''Come to our workshop to learn about:''' * ESA's Gaia mission,which was launched in Dec 2013 * results of the commissioning of the satellite * the first potential alerts on sup..." wikitext text/x-wiki '''Come to our workshop to learn about:''' * ESA's Gaia mission,which was launched in Dec 2013 * results of the commissioning of the satellite * the first potential alerts on supernovae and other transients from Gaia * results of the first alerts verification observations * potential science to be done with Gaia transients (e.g. supernovae, TDE, microlensing, CVs, young stellar objects, GRBs) * organisation of the follow-up for Gaia alerts * how to get involved '''Come to our workshop to contribute:''' * with your experience in science of transients * by presenting your results on surveying the sky for transients * showing what can potentially be done with the Gaia data * presenting your follow-up facility ready for Gaia alerts Gaia is the cornerstone mission of the European Space Agency, successfully launched in December 2013. Its main goal is to map the entire Galaxy, but thanks to repetitive observations of the entire sky it also acts as a unique time-domain space survey, suitable for real-time detections of transients. In recent years the astronomy of transient phenomena has became a very vivid area of research. Gaia will join to numerous current large-scale surveys like PTF, PANSTARRS, CRTS, SkyMapper, OGLE, LOFAR, which are aiming at delivering transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to supernovae and orphan Gamma Ray Bursts. However, without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost. It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. Gaia Science Alerts Workshops (GSAW) are organised annually since 2010. Their main goal has been, first, to keep the astronomical community informed and updated about the progress of the preparation and eventually the operation of the alert detection procedures within the Gaia data processing pipeline. The workshops have been acting as a platform for sharing experience from researching across the diverse transient phenomena, including supernovae, tidal disruption events, cataclysmic variables, microlensing events, young stellar object, R Corona Borealis-type stars and others. The workshops has been also facilitating organising the network of follow-up observatories, comprising of small and medium-sized telescopes from around the globe. All those goals are also to be achieved in the 2014 edition of the GSAW, however, the main difference this year is that we now have the Gaia satellite successfully launched and operational! By the time of the workshop in September, the mission should commence its nominal operation and we expect to have some first alerts already detected and published to the astronomical community. We should also have some first results to show and discuss from the extensive alerts verification campaign, which are currently being arranged on numerous spectroscopic and photometric facilities around the world. In September the mission should be well on track and there should be already some understanding on its performance, especially based on the commissioning period during which the Ecliptic Poles would be observed. At the workshop we will also hear the news from currently on-going transient surveys in their multi-wavelength and multi-messenger range and on their potential synergy with Gaia. Please accept this cordial invitation to participate in the Gaia Science Alerts Workshop 2014 in Warsaw, Poland, 9-12 September 2014. Let us together celebrate the successful start of the Gaia mission as well as Poland becoming a new member of ESA. The workshop will be supported financially via the European Commission OPTICON grant. There will be no registration fee. c13fe5d94160c79c5f3cae3247444488395d2510 1699 1698 2014-03-25T05:06:31Z Lukasz 2 wikitext text/x-wiki '''Come to our workshop to learn about:''' * ESA's Gaia mission,which was launched in Dec 2013 * results of the commissioning of the satellite * the first potential alerts on supernovae and other transients from Gaia * results of the first alerts verification observations * potential science to be done with Gaia transients (e.g. supernovae, TDE, microlensing, CVs, young stellar objects, GRBs) * organisation of the follow-up for Gaia alerts * how to get involved '''Come to our workshop to contribute:''' * with your experience in science of transients * by presenting your results on surveying the sky for transients * showing what can potentially be done with the Gaia data * presenting your follow-up facility ready for Gaia alerts ---- Gaia is the cornerstone mission of the European Space Agency, successfully launched in December 2013. Its main goal is to map the entire Galaxy, but thanks to repetitive observations of the entire sky it also acts as a unique time-domain space survey, suitable for real-time detections of transients. In recent years the astronomy of transient phenomena has became a very vivid area of research. Gaia will join to numerous current large-scale surveys like PTF, PANSTARRS, CRTS, SkyMapper, OGLE, LOFAR, which are aiming at delivering transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to supernovae and orphan Gamma Ray Bursts. However, without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost. It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. Gaia Science Alerts Workshops (GSAW) are organised annually since 2010. Their main goal has been, first, to keep the astronomical community informed and updated about the progress of the preparation and eventually the operation of the alert detection procedures within the Gaia data processing pipeline. The workshops have been acting as a platform for sharing experience from researching across the diverse transient phenomena, including supernovae, tidal disruption events, cataclysmic variables, microlensing events, young stellar object, R Corona Borealis-type stars and others. The workshops has been also facilitating organising the network of follow-up observatories, comprising of small and medium-sized telescopes from around the globe. All those goals are also to be achieved in the 2014 edition of the GSAW, however, the main difference this year is that we now have the Gaia satellite successfully launched and operational! By the time of the workshop in September, the mission should commence its nominal operation and we expect to have some first alerts already detected and published to the astronomical community. We should also have some first results to show and discuss from the extensive alerts verification campaign, which are currently being arranged on numerous spectroscopic and photometric facilities around the world. In September the mission should be well on track and there should be already some understanding on its performance, especially based on the commissioning period during which the Ecliptic Poles would be observed. At the workshop we will also hear the news from currently on-going transient surveys in their multi-wavelength and multi-messenger range and on their potential synergy with Gaia. Please accept this cordial invitation to participate in the Gaia Science Alerts Workshop 2014 in Warsaw, Poland, 9-12 September 2014. Let us together celebrate the successful start of the Gaia mission as well as Poland becoming a new member of ESA. The workshop will be supported financially via the European Commission OPTICON grant. There will be no registration fee. 4fc01dc93b25c9d9ff9a68dd1ee0f2acdd580e97 1700 1699 2014-03-25T05:06:51Z Lukasz 2 wikitext text/x-wiki '''Come to our workshop to learn about:''' * ESA's Gaia mission,which was launched in Dec 2013 * results of the commissioning of the satellite * the first potential alerts on supernovae and other transients from Gaia * results of the first alerts verification observations * potential science to be done with Gaia transients (e.g. supernovae, TDE, microlensing, CVs, young stellar objects, GRBs) * organisation of the follow-up for Gaia alerts * how to get involved '''Come to our workshop to contribute:''' * with your experience in science of transients * by presenting your results on surveying the sky for transients * showing what can potentially be done with the Gaia data * presenting your follow-up facility ready for Gaia alerts ---- Gaia is the cornerstone mission of the European Space Agency, successfully launched in December 2013. Its main goal is to map the entire Galaxy, but thanks to repetitive observations of the entire sky it also acts as a unique time-domain space survey, suitable for real-time detections of transients. In recent years the astronomy of transient phenomena has became a very vivid area of research. Gaia will join to numerous current large-scale surveys like PTF, PANSTARRS, CRTS, SkyMapper, OGLE, LOFAR, which are aiming at delivering transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to supernovae and orphan Gamma Ray Bursts. However, without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost. It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. Gaia Science Alerts Workshops (GSAW) are organised annually since 2010. Their main goal has been, first, to keep the astronomical community informed and updated about the progress of the preparation and eventually the operation of the alert detection procedures within the Gaia data processing pipeline. The workshops have been acting as a platform for sharing experience from researching across the diverse transient phenomena, including supernovae, tidal disruption events, cataclysmic variables, microlensing events, young stellar object, R Corona Borealis-type stars and others. The workshops has been also facilitating organising the network of follow-up observatories, comprising of small and medium-sized telescopes from around the globe. All those goals are also to be achieved in the 2014 edition of the GSAW, however, the main difference this year is that we now have the Gaia satellite successfully launched and operational! By the time of the workshop in September, the mission should commence its nominal operation and we expect to have some first alerts already detected and published to the astronomical community. We should also have some first results to show and discuss from the extensive alerts verification campaign, which are currently being arranged on numerous spectroscopic and photometric facilities around the world. In September the mission should be well on track and there should be already some understanding on its performance, especially based on the commissioning period during which the Ecliptic Poles would be observed. At the workshop we will also hear the news from currently on-going transient surveys in their multi-wavelength and multi-messenger range and on their potential synergy with Gaia. Please accept this cordial invitation to participate in the Gaia Science Alerts Workshop 2014 in Warsaw, Poland, 9-12 September 2014. Let us together celebrate the successful start of the Gaia mission as well as Poland becoming a new member of ESA. The workshop will be supported financially via the European Commission OPTICON grant. There will be no registration fee. 5e9525dab404d9a0c37bcd842a4a13e5ad806ee3 0 203 1701 1628 2014-03-25T06:08:49Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 96cba6bbec75ea2c9144d7cf56c127da8e22c0dc 0 203 1702 1701 2014-03-25T06:09:16Z Lukasz 2 /* Information about the requirements */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 0e87c4d4da43e84e3b8b7748009b567bc51c92be 1703 1702 2014-03-25T06:19:55Z Lukasz 2 /* Status of the partners preparing for the Gaia Alerts verification */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All == Test no 5 == Initiated 14/11/2013 Target: * iPTF13ebh supernova Ia == Test no 6 == Initiated 24/01/2014 Targets: * 2014J supernova Ia in nearby M82 galaxy * ASASSN-14ae, candidate for TDE, [http://www.astronomerstelegram.org/?read=5831] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK ad1b734a48c3da831db5d55037cfcc07785825c4 1704 1703 2014-03-25T06:21:24Z Lukasz 2 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK e4d5789ccd49642a9ea15a470d35e09cdcad0a0f 1709 1704 2014-03-25T06:29:29Z Lukasz 2 /* Status of the partners preparing for the Gaia Alerts verification */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK a55f70250fab611824f8e134d1a919251e423436 1710 1709 2014-03-25T06:31:25Z Lukasz 2 /* Tubitak Turkey */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov + ? * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: manual data upload within 24h Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 2b2e896cbfaa548997e8c73b9a5934e8474b806c 1711 1710 2014-03-25T06:33:33Z Lukasz 2 /* Tubitak Turkey */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm Status: <span style="color:#0000ff">manual data upload within 24h</span> Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 9fd7434712f6c8267be409bdf9ae60a2523693b8 1712 1711 2014-03-25T06:34:03Z Lukasz 2 /* Tubitak Turkey */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="background:#0000ff">manual data upload within 24h</span></big> Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 15edd127f21a77b32a87a0f5172a4a97870bae9f 1713 1712 2014-03-25T06:34:27Z Lukasz 2 /* Tubitak Turkey */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector Status: automated data upload ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 7d85bfc8bd8946ec69ce21f9609d839fb201bf8d 1714 1713 2014-03-25T06:36:33Z Lukasz 2 /* ASV Serbia */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados (szabados konkoly.hu) * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled Status: automated data upload ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic Status: automated data upload ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC Status: manual data upload. Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade) ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm Status: automated data upload === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK 5b7615b9cc337cb32b4421d27d710104fd255017 1715 1714 2014-03-25T06:41:56Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Loiano, Bologna, Italy * 1.5m * '''Status: ''' automated data upload ==== Asiago==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Padova, Italy * 1.82m ==== APT2==== * Contact person: Gisella Clementini (gisella.clementini oabo.inaf.it) * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien ==== TNT ==== * Contact person: Anna Piersimoni (piersimoni oa-teramo.inaf.it) * Location: Teramo, Italy, * 72cm Ritchey-Cretien ==== Belgian Mercatore ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Palma (Swiss time) * 1.2m ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Name and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca) ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade) ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer (laurent.eyer unige.ch) * La Silla, Chile * 1.2m ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK c3a5f477402223e75b6f8542dd7d273d51117dcc 1716 1715 2014-03-25T06:46:08Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. c18544f47b98faedb410230973dd8a6802be0074 1717 1716 2014-03-25T06:54:06Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. 05f1f5d5784f307a40edc01bd9426f442258cced 1721 1717 2014-03-26T23:38:10Z Lukasz 2 /* NORTH */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> Small FoV: problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. 7478beb7c58a9838f53cb03ba910449f922a05d1 1722 1721 2014-03-27T19:42:11Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. 0aa1ff763773086c71677111ee25f4f7293489b5 1723 1722 2014-03-28T20:06:33Z Lukasz 2 /* NORTH */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. 75e1e991e1105569fc415399de399ac9c686942d 1724 1723 2014-03-29T00:02:17Z Lukasz 2 /* Belgian Mercatore */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. 0a13ba410a7b7f469c9a9498cd280e404595509e 1734 1724 2014-05-26T14:51:21Z Gsawgwikiadmin 1 wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 12045e6beb6c4c325406b558d006b9593bd88211 1735 1734 2014-05-26T14:52:12Z Gsawgwikiadmin 1 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 491935c7251a293a3667fc4dc6513efab6047993 0 235 1705 2014-03-25T06:21:26Z Lukasz 2 Created page with "== Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright S..." wikitext text/x-wiki == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All == Test no 5 == Initiated 14/11/2013 Target: * iPTF13ebh supernova Ia, == Test no 6 == Initiated 24/01/2014 Targets: * 2014J supernova Ia in nearby M82 galaxy * ASASSN-14ae, candidate for TDE, [http://www.astronomerstelegram.org/?read=5831] db8880680a24ba35d72960d4289054fc788b3095 1706 1705 2014-03-25T06:26:45Z Lukasz 2 wikitext text/x-wiki == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183], [http://www.astronomerstelegram.org/?read=5245 ATel#5245 with results of the follow-up] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All == Test no 5 == Initiated 14/11/2013 Target: * iPTF13ebh supernova Ia, [http://www.astronomerstelegram.org/?read=5926 ATel#5926 with the follow-up results] [http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=25461 LC] == Test no 6 == Initiated 24/01/2014 Targets: * 2014J supernova Ia in nearby M82 galaxy * ASASSN-14ae, candidate for TDE, [http://www.astronomerstelegram.org/?read=5831] 8b430a291900f850c2809337acb3c6de0d662aa2 1707 1706 2014-03-25T06:27:53Z Lukasz 2 wikitext text/x-wiki == Test no 1 == Initiated 29/10/2012 Targets for the North: * CSS121011:163803+372814 [http://nunuku.cacr.caltech.edu/catalina/20121011/1210111380724113233.html] - rel.bright SN Ia * CSS121015:004244+132827 [http://voeventnet.caltech.edu/feeds/ATEL/CRTS/1210151120044133047.atel.html] - Super-luminous SN * CSS121026:164652+565105 [http://nunuku.cacr.caltech.edu/catalina/20121026/1210261570504105230.html] - SN Ia Targets for the South: * OGLE-2012-SN-06 [http://ogle.astrouw.edu.pl/ogle4/transients/transients.html] - possibly a Super-luminous SN Participants: PIRATE, Belgian, pt5m, Loiano, Asiago, GROND ==Test no 2 == Initiated 3/07/2013 Targets: * ASASSN-13aw [http://www.astronomerstelegram.org/?read=5183], [http://www.astronomerstelegram.org/?read=5245 ATel#5245 with results of the follow-up] * MASTER OT J174816.22+501723.3 [http://www.astronomerstelegram.org/?read=5182] * ASASSN-13ba (giant M-flare?, 13mag) * ASASSN-13ax (bright CV, 13mag) Participants: Serbia, Bulgaria, Vienna, pt5m, Konkoly == Test no 3 == Initiated 27/9/2013 [[File:ASASSN-13dd-RTT150-r.png|right|200px|frame|ASASSN-13dd captured by RTT150 on 29.Sep 2013]] Target: * ASASSN-13dd supernova about 15 mag Participants: Turkey, Serbia == Test no 4 == Initiated 11/10/2013 Target: * ASASSN-13dl young supernova, 16.5 mag Participants: All == Test no 5 == Initiated 14/11/2013 Target: * iPTF13ebh supernova Ia, [http://www.astronomerstelegram.org/?read=5926 ATel#5926 with the follow-up results] [http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=25461 follow-up light curve] == Test no 6 == Initiated 24/01/2014 Targets: * 2014J supernova Ia in nearby M82 galaxy, [http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=25462 follow-up light curve] * ASASSN-14ae, candidate for TDE, [http://www.astronomerstelegram.org/?read=5831], [http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=25463 follow-up light curve], 4b4cfa94f9f7b24b76c872cecf09911c188039b7 0 11 1708 1330 2014-03-25T06:28:47Z Lukasz 2 /* Preparations for the verification phase */ wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Verification:tests|Test observing campaigns and results]] [[Status of the verification partners]] ---- Useful link with list of telescopes of the world: [http://www.eso.org/~ndelmott/obs_sites.html] 746b1911543f05487fe53132f0ba8297d76bd541 1730 1708 2014-05-05T07:54:12Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Verification:tests|Test observing campaigns and results]] [[Status of the verification partners]] ---- = Allocated observing time = == SAO 1.9m == * 16-30 September 2014 (TBC) * Steve Potter, local observers, Krystian Ilkiewicz (Poland, helps with data reductions) * Spectroscopy * V<17 mag == Loiano 1.5m == * 16-30 September 2014 (TBC) * Gisella Clementini, Krzysztof Ulaczyk, Michal Pawlak, Lukasz Wyrzykowski, students from Poland and Italy * Spectroscopy and photometry 579c2f4f38bc0da605aba875d496d56dae1a8b0a 1731 1730 2014-05-05T19:45:32Z Gsawgwikiadmin 1 /* Allocated observing time */ wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Verification:tests|Test observing campaigns and results]] [[Status of the verification partners]] ---- = Allocated observing time = == SAO 1.9m == * 16-30 September 2014 (TBC) * Steve Potter, local observers, Krystian Ilkiewicz (Poland, helps with data reductions) * Spectroscopy * V<17 mag == Loiano 1.5m == * 16-30 September 2014 (TBC) * Gisella Clementini, Krzysztof Ulaczyk, Michal Pawlak, Lukasz Wyrzykowski, students from Poland and Italy * Primarily photometry == Asiago 1.8m == * 16 September until ?? * People? * Primarily spectroscopy 0897b49d04fd4232f74a618a1e8cc1c003c4918d 1733 1731 2014-05-26T14:49:27Z Gsawgwikiadmin 1 /* Loiano 1.5m */ wikitext text/x-wiki '''<big>Concise pack of information is available in the [[Media:verificationbrochure.pdf | Verification brochure]]</big>''' ---- The main aim of the Science Alerts Verification Phase (SAVP) is to verify the robustness of the issued alerts and confirm them with a dedicated network of follow-up telescopes operating in a ''Target of Opportunity'' (ToO) mode. The verification observations should be carried out both photometrically (imaging) and spectroscopically in order to, e.g. confirm the presence of the detected new object, or to confirm or fine-tune the classification of the alert. The verification phase should reveal all necessary adjustments which have to be done to the detection and classification algorithms to assure the best and the most robust performance later on. The verification phase could last for about 3 months and is planned to take place after around 3-6 months after receiving the first Gaia data to assure there is enough historical data available for most of the objects, and to allow for shake-down of the Gaia Initial Data Treatment (IDT). Some areas (close to the nodes of the scanning pattern) will have enough observations accumulated to allow for an earlier start of the alerting pipeline, as long as the GAIA data flow is operating smoothly. In principle, some pre-launch preparation could take place in the areas of very dense Gaia sampling. This could include gathering all useful information about the objects in these regions, both from existing catalogues and accompanied by new observations. This could include variability classification and spectral type classification to test recovery of known candidate (potential) transient sources, as well as likely contaminants. [[File:ScienceAlerts-timeline.png|700pix]] The Science Alerts Verification Phase will be conducted mainly under umbrella of GBOG (Ground Based Observations for Gaia), however we encourage other groups of astronomers to join this effort as early as possible. Early involvement in the alerts observations can result in establishing a good connection with the Gaia alerts stream when they become fully public. '''If you have a telescope and would like get involved in the Gaia alerts verification, please contact [[User:Lukasz| Lukasz Wyrzykowski]]''' == Photometric Calibrations Server == Please refer to [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up#Gaia_Science_Alerts_Follow-up_Server Gaia Science Alerts Follow-up Server] page for details on uniform calibration procedures = Preparations for the verification phase = We are now at the preparation stage for the verification. There still time to join the Gaia Follow-Up Network for Transient Objects (Gaia-FUN-TO). Each potential partner must complete a series of tests before the actual verification phase begins. [[Verification:tests|Test observing campaigns and results]] [[Status of the verification partners]] ---- = Allocated observing time = == SAO 1.9m == * 16-30 September 2014 (TBC) * Steve Potter, local observers, Krystian Ilkiewicz (Poland, helps with data reductions) * Spectroscopy * V<17 mag == Loiano 1.5m == * 16-30 September 2014 (TBC) * Gisella Clementini, Krzysztof Ulaczyk, Michal Pawlak, Lukasz Wyrzykowski, students from Warsaw, Bologna and Cambridge. * Primarily photometry == Asiago 1.8m == * 16 September until ?? * People? * Primarily spectroscopy 08e3d6da95c1a8fb61efb6ebb624dd545e40422f 0 86 1718 1684 2014-03-25T22:47:12Z Lukasz 2 wikitext text/x-wiki List of catalogues to be used for cross-matching Gaia Science Alerts sources: * SDSS * 2MASS * NED * ASAS [http://www.astrouw.edu.pl/asas/] - long term photometry data in I and V. Whole sky (N+S), down to 14mag * OGLE [http://ogle.astrouw.edu.pl] - long term photometry data in I and V. Bulge and Magellanic Clouds only * INTEGRAL [http://arxiv.org/abs/0910.1704] - Gamma-ray sources, all sky, data available for download [http://integral.esac.esa.int/isda/] * WISE all sky infrared catalogue, simple cuts can help distinguish SN from AGNs, RCrB from EB, YSO, etc. (e.g. [http://adsabs.harvard.edu/abs/2012ApJ...744..130K], [http://adsabs.harvard.edu/abs/2012A%26A...539A..51T], [http://adsabs.harvard.edu/abs/2013ApJ...772...26A]) e662274c3447debb88c2227c3b4b5e3ebfe9f37c 0 234 1719 1700 2014-03-26T02:35:18Z Lukasz 2 wikitext text/x-wiki '''Come to our workshop to learn about:''' * ESA's Gaia mission,which was launched in Dec 2013 * results of the commissioning of the satellite * the first potential alerts on supernovae and other transients from Gaia * results of the first alerts verification observations * potential science to be done with Gaia transients (e.g. supernovae, TDE, microlensing, CVs, young stellar objects, GRBs) * organisation of the follow-up for Gaia alerts * how to get involved '''Come to our workshop to contribute:''' * with your experience in science of transients * by presenting your results on surveying the sky for transients * showing what can potentially be done with the Gaia data * presenting your follow-up facility ready for Gaia alerts ---- Gaia is the cornerstone mission of the European Space Agency, successfully launched in December 2013. Its main goal is to map the entire Galaxy, but thanks to repetitive observations of the entire sky it also acts as a unique time-domain space survey, suitable for real-time detections of transients. In recent years the astronomy of transient phenomena has became a very vivid area of research. Gaia will join numerous current large-scale surveys like PTF, PANSTARRS, CRTS, SkyMapper, OGLE, LOFAR, which are aiming at delivering transient objects corresponding to a wide range of astrophysical phenomena, from solar system objects, through new types of stellar variability and signatures of exoplanets, to supernovae and orphan Gamma Ray Bursts. However, without prompt and appropriate follow-up observations, much of the scientific potential of these new discoveries will be lost. It becomes crucial for transient astronomy that the new phenomena are rapidly observed with small and medium size telescopes and the data are analysed quickly to share the knowledge. Gaia Science Alerts Workshops (GSAW) has been organised annually since 2010. The main goal has been, first, to keep the astronomical community informed and updated about the progress of the preparation and eventually the operation of the alert detection procedures within the Gaia data processing pipeline. The workshops have acted as a platform for sharing experience from researching into diverse transient phenomena, including supernovae, tidal disruption events, cataclysmic variables, microlensing events, young stellar objects, R Corona Borealis-type stars and others. The workshops have also helped us to organise a network of follow-up observatories, comprising of small and medium-sized telescopes from around the globe. All those goals are also to be achieved in the 2014 edition of the GSAW, however, the main difference this year is that we now have the Gaia satellite successfully launched and operational! By the time of the workshop in September, the mission should commence its nominal operation and we expect to have some first alerts already detected and published to the astronomical community. We should also have some first results to show and discuss from the extensive alerts verification campaign, which are currently being arranged on numerous spectroscopic and photometric facilities around the world. In September the mission should be well on track and there should be already some understanding on its performance, especially based on the commissioning period during which the Ecliptic Poles would be observed. At the workshop we will also hear the news from currently on-going transient surveys in their multi-wavelength and multi-messenger range and on their potential synergy with Gaia. Please accept this cordial invitation to participate in the Gaia Science Alerts Workshop 2014 in Warsaw, Poland, 9-12 September 2014. Let us together celebrate the successful start of the Gaia mission as well as Poland becoming a new member of ESA. The workshop will be supported financially via the European Commission OPTICON grant. There will be no registration fee. 74a926272f1cb607cde278b21287513eac0c457f 0 226 1720 1675 2014-03-26T23:33:06Z Lukasz 2 /* Workshop Organizing Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Szymon Kozlowski LOC: * Zuzanna Kostrzewa-Rutkowska * Alicja Rynkiewicz * Lukasz Wyrzykowski * Szymon Kozlowski 027430e5471a1c544e88e635227ee567c7986add 1725 1720 2014-04-08T11:22:53Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Nic Walton * Szymon Kozlowski * Heather Campbell * Morgan Fraser * Nadejda Blagorodnova LOC: * Zuzanna Kostrzewa-Rutkowska * Alicja Rynkiewicz * Lukasz Wyrzykowski * Szymon Kozlowski d97f9d385cbf0bb9dcb43359e5d64e1b7be53f03 1739 1725 2014-07-07T20:46:40Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Nic Walton * Szymon Kozlowski * Heather Campbell * Morgan Fraser * Nadejda Blagorodnova LOC: * Zuzanna Kostrzewa-Rutkowska * Alicja Rynkiewicz * Lukasz Wyrzykowski * Szymon Kozlowski * Monika Sitek 767442a976790ace85d67c2210fe8df48b44058c 1740 1739 2014-07-08T10:05:04Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Nic Walton * Szymon Kozlowski * Heather Campbell * Morgan Fraser * Nadejda Blagorodnova LOC: * Zuzanna Kostrzewa-Rutkowska * Alicja Rynkiewicz * Lukasz Wyrzykowski * Szymon Kozlowski * Krzysztof Rybicki * Monika Sitek bdff84487b95e1ca0d2388211c6c35aa8b0b95f5 6 236 1726 2014-04-27T20:11:38Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 237 1727 2014-04-27T20:14:45Z Gsawgwikiadmin 1 Created page with "*[http://www.astrouw.edu.pl/~wyrzykow/Gaia_2014-poster.pdf 2MB PDF] ---- Poster created by Amanda Smith, Institute of Astronomy, Cambridge" wikitext text/x-wiki *[http://www.astrouw.edu.pl/~wyrzykow/Gaia_2014-poster.pdf 2MB PDF] ---- Poster created by Amanda Smith, Institute of Astronomy, Cambridge 525f4a047c35162a8f3ac98c0a0b8e8ee7af6122 1728 1727 2014-04-27T20:15:32Z Gsawgwikiadmin 1 wikitext text/x-wiki *[http://www.astrouw.edu.pl/~wyrzykow/Gaia_2014-poster.pdf Download here (2MB PDF)] [[File:Poster2014.jpg|right]] ---- Poster created by Amanda Smith, Institute of Astronomy, Cambridge 5038a9a14a63fe3205253abe3f45f8ee3cefcda0 1729 1728 2014-04-27T20:15:43Z Gsawgwikiadmin 1 wikitext text/x-wiki *[http://www.astrouw.edu.pl/~wyrzykow/Gaia_2014-poster.pdf Download here (2MB PDF)] [[File:Poster2014.jpg|right|300px]] ---- Poster created by Amanda Smith, Institute of Astronomy, Cambridge 5769e8a756e89edafbfb7fbcff03b743edc24dae 0 214 1732 1682 2014-05-09T09:34:44Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 57b6557c9085af376852efe0ddcb4d9791b39f61 0 233 1736 1697 2014-06-22T20:42:09Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!'''</big> [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA 1a4069d0dc3845f0d24d457407de7b2f2d61e326 1737 1736 2014-06-24T10:36:38Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK 1c06f6341d52680273198ed3f51b7fa6c82ad6eb 1738 1737 2014-07-05T19:36:34Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands f3fd90bedbcdd79ac3e225d756393fe01fa876fb 0 227 1741 1685 2014-07-08T14:20:40Z Gsawgwikiadmin 1 /* Accommodation */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] a2ab065116fba596ddf037747d2dba656e3c7721 1742 1741 2014-07-08T14:24:54Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] c8d51da50441f92f26fbaadec56d3b7ffa18af8d 1743 1742 2014-07-08T14:25:08Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] [[File:map.png|600px]] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] b4c5d56fabb06a7b2ef4e8322c4c18742c22bca0 1744 1743 2014-07-08T14:25:24Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] d4a22ee27497c40ca7aea0ab92287a654aae1183 1745 1744 2014-07-08T14:27:22Z Gsawgwikiadmin 1 /* Accommodation */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl] Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 80f14c6ca07da44e1ad72e3892ecf2a3512f33be 1746 1745 2014-07-08T14:27:50Z Gsawgwikiadmin 1 wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] c6a44c40aea5d1801bb0c8ee4eaab73c14f812ae 1747 1746 2014-07-08T14:31:44Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 12080b7a3c0215915b3cf79e654ba96940e10dcf 1748 1747 2014-07-08T14:34:48Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk to the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] fb46eb616ae42aa05af27deab2438d4c141dcb63 1749 1748 2014-07-08T14:36:22Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk to the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 6024ceacc6064640ddccd63f242aea77753f6894 1750 1749 2014-07-08T14:36:42Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk to the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] b9720505d4bc016159062c20456cd7b1f889ea92 1751 1750 2014-07-08T14:38:48Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] db28d5d33e157fb7e80a94f1fab142fd4582d384 0 227 1752 1751 2014-07-08T14:39:22Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the vicinity: * [http://www.accorhotels.com/pl/hotel-3378-sofitel-warsaw-victoria/index.shtml SOFITEL] * [http://www.hotelharenda.com.pl/ Harenda] Hotels situated up to 20 minutes away from the workshop venue: * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 08546723c7b0f5945bbff212a2f7cd4a82ab4e31 1753 1752 2014-07-08T16:00:48Z Zuzanna 36 /* Accommodation */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the city centre: * [http://www.hiltoneasteurope.com/ Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] * [http://www.lazienkowski.pl/ Łazienkowski] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 8ba6e70f6f1e53058b650a6ad239e7b321a116e5 1754 1753 2014-07-08T16:03:27Z Zuzanna 36 /* Accommodation */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin (Ost), Amsterdam, Prague and Vienna (Wien Simmering). Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the city centre: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] * [http://www.lazienkowski.pl/ Łazienkowski] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 06170297bb763af15233fcdf0dd9dbecb8dcb30f 1756 1754 2014-07-09T08:37:45Z Zuzanna 36 /* By Train */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Train Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the city centre: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] * [http://www.lazienkowski.pl/ Łazienkowski] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] db5cb676ee9c45aa58db1d4099a8223181a65058 1757 1756 2014-07-09T08:41:44Z Zuzanna 36 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Railway Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the plenary part of the workshop will take place in room 316, the main auditorium. On the 12 September the splinters will take place in two smaller rooms nearby. [[File:buw-foto.jpg]] [[File:buw-sal.jpg|250px| Main auditorium ]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the city centre: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] * [http://www.lazienkowski.pl/ Łazienkowski] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 5cfb8359e2c28741a1418e0ea7ccea0bc15fd808 0 233 1755 1738 2014-07-08T21:19:20Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France e09764b1070d5674b3338f934d7d38c240613c97 1758 1755 2014-07-09T14:29:14Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK f819c26f075233989a7e6113afb6641a91ec3c96 1759 1758 2014-07-12T15:28:20Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa e45716f6afd54106224329c1dbebb66fbe864c64 1776 1759 2014-07-16T10:19:51Z Zuzanna 36 /* List of registered participants: */ wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands 090af065c7744459a54a2e0a1f1e3c18aa13894d 1778 1776 2014-07-21T11:32:32Z Zuzanna 36 /* List of registered participants: */ wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany d895d079c2f5d53a98c423b9efc29885f173c049 1779 1778 2014-07-23T08:52:54Z Lukasz 2 /* List of registered participants: */ wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic af8572d2afd3152c8d0ffab26d570c71b2a01a66 1781 1779 2014-07-24T20:41:16Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK 8b4f7b40e2a214e0d511b3a022a05c2fed8bbdf7 1783 1781 2014-07-27T20:46:16Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland 7f1d21d6bd43bcb4b0183df8a62f1ce64ce19164 1784 1783 2014-07-28T14:08:26Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland f8591438ee3d7e85b46bd305325deae9ce06e534 1785 1784 2014-07-29T15:30:46Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK d864e851be87ed4d22ee874b14a984688fd6a146 1786 1785 2014-07-29T15:42:55Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia b96186038070e8e5ba362feb7a4b73bc2a64b7ac 1787 1786 2014-07-30T09:04:11Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France 2bdd0ff93dcfedc10ed55b8d33fb7693a0761f4e 1789 1787 2014-07-30T10:36:26Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK fdc39d69a23cb63374edbf3f68d11853685d750e 1794 1789 2014-07-30T14:09:46Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria 6dfdbabdb7e938785a77291984dda30c463d9ed2 1795 1794 2014-07-30T15:04:52Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK a3c4c5963b281b895b779a69cb13e54bdbe2b980 1796 1795 2014-07-30T15:48:50Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland 1c293dc07f21ecb80c7eaff8540f46a08dae79aa 1797 1796 2014-07-30T20:06:11Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK 46b13335ec338825d39ade70fd0c4b047fc7b728 1798 1797 2014-07-30T20:48:01Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK f9f06bb018e7add7f9f59b6a6e0344ac9a29fa24 1799 1798 2014-07-31T09:20:18Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland 39c9f98ded25e0d1f7f959beb12f6dda5beb5fec 1800 1799 2014-07-31T11:26:13Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland 1431808043db2133a8dfb1c913b8b1b955b95996 1801 1800 2014-07-31T13:20:20Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland 5c1ca152aec42890cff89f6dcb8aa93d28308bdd 0 17 1760 1462 2014-07-13T13:45:04Z Sth 6 /* Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: here 6b18a11553be1b9e94dfb4868b5c9885cbebc8f2 1761 1760 2014-07-13T13:46:37Z Sth 6 /* Coordination of follow-up spectroscopy and photometry */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] 9d934531b346726c23867a87c0124dc01cbed535 0 238 1762 2014-07-13T14:04:06Z Sth 6 Created page with "On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic'' observing runs for the upcoming semesters. This page will be amended as more follow-up run..." wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic'' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-style: solid; border-width: 20px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} PIs : Hodgkin (INT - 15 nights), Wevers (INT - ), Fraser (WHT - ), Campbell (INT - 7 nights, WHT - 7 nights, Mercator - 15 nights) Observing Rota: Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). Date Telescope Observers a9268bdf9f6a93dedf12156def5d269f0057d321 1763 1762 2014-07-13T14:28:05Z Sth 6 /* 2014B Observing Time Awarded */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic'' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} PIs : Hodgkin (INT - 15 nights), Wevers (INT - ), Fraser (WHT - ), Campbell (INT - 7 nights, WHT - 7 nights, Mercator - 15 nights) ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || Jonker || N4 || INT || IDS || TWevers |- | 21-24 Aug || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || Hodgkin || P14 || INT || IDS || |- | 29-30 Sep || Fraser || P29 || WHT || ACAM || |- | 28 Oct || Fraser || P29 || WHT || ISIS || |- | 15-18 Nov || Wevers || N7 || INT || IDS || |- | 27-29 Nov || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || Campbell || ITP2 || INT || IDS || |} f22e59c2bb1337846c9ad74f31cdff7b2984da80 1764 1763 2014-07-13T14:56:59Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic'' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} PIs : Hodgkin (INT - 15 nights), Wevers (INT - ), Fraser (WHT - ), Campbell (INT - 7 nights, WHT - 7 nights, Mercator - 15 nights) ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || TWevers |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || ISIS + ACAM || |} b417c23e9ebe0c18f4a1c034cb55ce4338372a1b 1765 1764 2014-07-13T15:06:22Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic'' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} PIs : Hodgkin (INT - 15 nights), Wevers (INT - ), Fraser (WHT - ), Campbell (INT - 7 nights, WHT - 7 nights, Mercator - 15 nights) ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |} a4af4c69ab7e10f116466127ffff5f3294d60248 1766 1765 2014-07-13T15:06:42Z Sth 6 /* 2014B Observing Time Awarded */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic'' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |} ccdbaeda36e7cff35b273d37dab29885f6dda1c9 1767 1766 2014-07-13T15:08:45Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |} 07948a38a626f347cd35c27955c7a6aaac1a280f 1768 1767 2014-07-13T15:10:18Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 7b375997eeb45ec35972bd333d18bda902bf3fa4 1769 1768 2014-07-14T11:13:42Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 0859466ee7bd0dbd9a53c2eb0bd6fef22f5fd25b 1770 1769 2014-07-14T11:19:19Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' ef29986ac25dad6a2372f9c4e1f89d8d35bf7627 1771 1770 2014-07-14T11:23:46Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 693ab24169c0e34142ae2e75c9fb48319a7b18eb 1772 1771 2014-07-14T11:25:59Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 2aa960268d485ac14a023daf54f0b2979223ae97 1773 1772 2014-07-14T11:35:01Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Dutch?'', ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Dutch?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 41491f3f4902966aa9d7a71cf87b8822609cc46a 1774 1773 2014-07-14T11:36:56Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} <!--- Comment ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Dutch?'', ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Dutch?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ---> |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' abcd80da6ce2fdb17b00d65ab13f7d6787db47cc 1775 1774 2014-07-14T11:37:58Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |} <!--- Comment ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Dutch?'', ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Dutch?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} ---> === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 23a8d5a8228960a3ae526fbf70a938bfc15535e4 1777 1775 2014-07-18T12:36:57Z Gsawgwikiadmin 1 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} <!--- Comment ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Dutch?'', ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Dutch?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} ---> === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 74cb656f45c73771d2bc5aceba870b430d2fec47 1782 1777 2014-07-25T11:17:54Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Dutch?'', ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Dutch?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' c0e87020ef3a20b69f5dd8f70919a01800287eca 1788 1782 2014-07-30T09:26:03Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''TWevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS ||''Campbell+NL'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Dutch?'', ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || "Van Velzen" |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || "Jonker?" |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' d1934a53d95f8f8aa1be16d98e71b017642019c1 1790 1788 2014-07-30T13:08:45Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || "Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Weevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || "Van Velzen" |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || "Jonker?" |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' c503149d922629dc3a3d6f1340d85886f06f4e07 1791 1790 2014-07-30T13:09:14Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Weevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || "Van Velzen" |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || "Jonker?" |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' a7b28f1d87de98e1b744f5451c47df9d3af7c908 1792 1791 2014-07-30T13:14:01Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Weevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Jonker?'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' d9dc4327482f3c275115241bee995285c49f8904 1793 1792 2014-07-30T13:14:35Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Jonker?'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' a6abe9097e8cb39851993ffd7cc3be192d099837 0 231 1780 1686 2014-07-23T10:53:44Z Lukasz 2 wikitext text/x-wiki The preliminary outline of the workshop: * 9.Sep, Tuesday, workshop commences in the afternoon * 10.Sep, Wednesday, full day, workshop dinner in the evening at Zacheta Art Gallery, can be combined with visiting the art exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!] * 11. Sep, Thursday, full day * 12. Sep, Friday, splinter sessions, hands-on, workshop closes after lunch 31bc1429761de5ae9dbb65817cc5d976c9bc617b 0 233 1802 1801 2014-07-31T16:20:14Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''31st July 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK 9af491397c8de4f3acd46bd1c948f168d9606a4d 1803 1802 2014-07-31T20:22:35Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK c2b27b2fbd5ced21721a0b9e6349d215edd66d96 1804 1803 2014-07-31T21:47:07Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK 10d74ba44ca8c5b55b6107620f19b9d39f586d08 1805 1804 2014-08-01T11:20:32Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy d73252df8115088bf371d50f35a95875fe98a052 1806 1805 2014-08-01T12:50:10Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland 6e9d0e92bf7ce85e635a4103d6b1f4bc9ca5b832 1807 1806 2014-08-01T16:18:07Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK 1a1c199270403d6187061562f1ad6001f6b7549a 1808 1807 2014-08-05T09:15:47Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK 2f476fb95649a2363cc4be9944406b9ce693e2e6 1809 1808 2014-08-07T20:08:22Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland 8f86902e8f4cb7034562c1c39430f59173ed9ebc 1812 1809 2014-08-08T20:19:51Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now open!''' [[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. </big> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge a40b4448ea20c6b723aa128f5399150bc3355270 1813 1812 2014-08-08T20:21:29Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed!'''</big> If you still feel like joining us, please email us. <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge 34906150728e4b712702f512ef4c38a3024b4b1b 1814 1813 2014-08-08T20:21:37Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed!'''</big> If you still feel like joining us, please email us. <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge 58ce0b6cc45524f9df55b1dc7d2ddac0b12bcbda 1815 1814 2014-08-08T20:21:47Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us. <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge 6296d1d9f8c4ce20765301f181d7be69dff71ff4 1816 1815 2014-08-08T20:22:04Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge bfacca6e0ae9a56caec038e0dcdadff3c6a643e1 1817 1816 2014-08-08T20:22:12Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> \*If you still feel like joining us, please email us asap! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge fe97b561cbf21048aa4fd007b898cd67ba213ec1 1818 1817 2014-08-08T20:22:20Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> "*"If you still feel like joining us, please email us asap! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge 71c29ca83cc32d8ec563a03a4b3d8a5b711b63ce 1819 1818 2014-08-08T20:22:31Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge bfacca6e0ae9a56caec038e0dcdadff3c6a643e1 1820 1819 2014-08-08T20:50:14Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland 5d751b0a74659bbe25acdc7beaf8c6b5b49414aa 1821 1820 2014-08-13T13:48:45Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland 10b4ed5f6155f073b56d173ba01cfd880f9fdb25 1822 1821 2014-08-15T18:37:45Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France 165b6b475c97014572dc53b7630b89ad29086de9 1823 1822 2014-08-15T21:09:34Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland 464957983b82e4e3951d1be79e09a6d9cbacd9ee 1824 1823 2014-08-18T08:59:18Z Zuzanna 36 /* List of registered participants: */ wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL 687bf6805c6d034e98f6f8f9de7931063e9deced 1825 1824 2014-08-18T18:21:55Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Ashish Mahabal, Caltech, USA #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL 58b57288bc021e4ffcd20707936e7a8b52ca41d9 1826 1825 2014-08-19T13:26:08Z Zuzanna 36 /* List of registered participants: */ wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Nicholas Walton, IoA, Cambridge, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL cc957198e1cafb1311c79f890048a0232f5a2c3e 1845 1826 2014-08-30T16:11:31Z Zuzanna 36 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Arne Henden, AAVSO, USA #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL 8a7415b004015cc68473c64e1001fcc44ed83d1a 1848 1845 2014-09-01T11:46:54Z Zuzanna 36 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL b682e40ac77e9e182f7466716e0e15e5de8d7cab 1849 1848 2014-09-02T10:07:04Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL #John Davies, Edinburgh, UK f4b540e7dc03d52d5d8c5de0dd6ad24fc4cf9998 1850 1849 2014-09-02T14:27:35Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL #John Davies, Edinburgh, UK #Igor Soszynski, OAUW, Poland d4abade9015d5d6070304a8d8fb3a01d133c144f 0 238 1810 1793 2014-08-08T10:58:13Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'', ''Rixon?'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Jonker postdoc?'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 22b5f8a7f0b13c06c5928c61ec8a57c9a84a48c8 1811 1810 2014-08-08T11:13:06Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon*?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Jonker postdoc?'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' c808f0a9f6da0595062ec60b4978efe1e4fc1678 1837 1811 2014-08-21T22:56:37Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon*?'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker?'', ''Rixon?'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat?'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Copperwheat?'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Jonker postdoc?'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 85d43dd4a3cce31815dbb9fb84c849bd4c558ec5 0 231 1827 1780 2014-08-19T22:22:03Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Commissioning |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |10:45 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Insera (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Sjoert van Velzen (Nijmegen) |TDEs |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- |colspan="4"|'''Friday 12 September 2014''' |''''NOTE CHANGE OF ROOM'''' | | |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |} d0f37b9dab10e4a523449f2abd3b73576126ef51 1828 1827 2014-08-19T22:23:46Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Commissioning |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |10:45 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Insera (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Sjoert van Velzen (Nijmegen) |TDEs |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- |colspan="3"|'''Friday 12 September 2014''' |''''NOTE CHANGE OF ROOM'''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |} bd0582c4323f70a60c2588e4aef676ee2347bf7f 1829 1828 2014-08-19T22:27:45Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Commissioning |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |10:45 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Insera (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Sjoert van Velzen (Nijmegen) |TDEs |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- |---- |colspan="3"|'''Friday 12 September 2014''' |''''NOTE CHANGE OF ROOM'''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 7b3535c2e18e51650c7d1c3c8c0aab6027c28c00 1830 1829 2014-08-19T22:29:08Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Commissioning |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |10:45 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Insera (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Sjoert van Velzen (Nijmegen) |TDEs |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} f54fd4e422bf9cef702948dc2edc6ae2dbf869c8 1831 1830 2014-08-20T05:24:12Z Zuzanna 36 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Commissioning |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |10:45 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Sjoert van Velzen (Nijmegen) |TDEs |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 10fddda0b001c99ebcca90797bdda023ed0a8656 1832 1831 2014-08-20T08:57:35Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Sjoert van Velzen (Nijmegen) |TDEs |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 32c216cb833b3c172471ef4b9b918898c278403c 1833 1832 2014-08-21T10:46:30Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} e2d406f000a6929e564efa713dac5c2a780b0b97 1834 1833 2014-08-21T10:53:45Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} d7708a3be40b9b8f91ab86949cd137f2aa6b5e6a 1835 1834 2014-08-21T10:54:22Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Arne Henden (AAVSO) |Citizen Science in the Age of GAIA |0:25 |---- |17:25 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:20 |---- |17:45 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 88f50cfc5bad3f19cbf3bf1be154cbc9c4fee4d7 1838 1835 2014-08-23T21:19:41Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:25 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 43e1c2e451d5e3ae9daa18f2d45f260fb89b6ec6 1839 1838 2014-08-25T20:49:55Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:25 |'''end of day 3''' | | |---- | | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |10:00 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:20 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:30 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:45 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |12:00 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:15 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:30 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 4eddb9ab127d75f7d36a0016d5008ae5304eec34 1840 1839 2014-08-29T10:36:44Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |''19:00'' |''Gerry Gilmore (Cambridge)'' |''Public Talk in the Copernicus Science Centre'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:05 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:15 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:30 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:45 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:00 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:15 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 00138555068c53050eca93da794e96dc9c578b1b 1841 1840 2014-08-29T10:37:46Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | |'''with optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the Copernicus Science Centre''' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:05 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:15 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:30 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:45 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:00 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:15 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} e8b26b6c57d3810b2069308ab983eeb4f34cb814 1842 1841 2014-08-29T13:28:54Z Zuzanna 36 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the Copernicus Science Centre''' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Nic Walton (Cambridge) |GREAT Network |0:15 |---- |09:45 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |10:05 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:15 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:30 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:45 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |12:00 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:15 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} fef15d13c30b1a9eb7c1eb768e03593c4febf0fa 1843 1842 2014-08-30T13:18:17Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the Copernicus Science Centre''' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:15 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:30 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |12:45 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} d112200e73a5909f484a75da4f7765da7b658af1 1844 1843 2014-08-30T13:20:02Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' | | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:15 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:30 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |12:45 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} b7092d25f82b0ed43e8f11109590503d6986b403 1846 1844 2014-09-01T09:10:44Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |'''price: 10 PLN per person''' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) |'''price: 190 PLN per person''' |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' (ticketed,free for workshop attendees) | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:15 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:30 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |12:45 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 0c3d04c67e75d78c442f067aa3cfdaa8b96c49c5 1847 1846 2014-09-01T09:57:20Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:15 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:30 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |12:45 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 5739e8f9557ce96eb0f8e3531001d7c91c20c92a 1851 1847 2014-09-02T18:49:29Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa |Geneva Observatory |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 73f94cd81b6aee09708031f4b890471b42243b56 6 239 1836 2014-08-21T10:54:51Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 231 1852 1851 2014-09-02T18:50:18Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 66efa905d1005eaf1acddacf3809cf40931936c8 1853 1852 2014-09-02T19:01:18Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[Media:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:15 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 8aa05a4bc085d76e9d71deb4dd83e33ca3fdbb48 1856 1853 2014-09-03T06:34:07Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[Media:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Kester Smith (Heidelberg) |Automated classification of Gaia sources |0:25 |---- |10:20 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:35 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:50 |'''coffee''' | |0:30 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |17:15 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} db868fc9e5709413a6b4c4e733d578a8266e70d0 1858 1856 2014-09-03T13:41:48Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[Media:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:30 |---- |17:00 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |09:55 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |10:20 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |11:55 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |17:00 |Gerry Gilmore (Cambridge) |OPTICON |0:15 |---- |17:10 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:40 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 5e7dd675342c8299ba451e780c4aac0988b2736b 1859 1858 2014-09-03T13:46:15Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[Media:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Gerry Gilmore (Cambridge) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 77e92bb9b7784c340d8c7db4ba67af9f816430ad 1860 1859 2014-09-03T15:13:03Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |Gerry Gilmore (Cambridge) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 4f665e0b0d4dee68248fb26d2ce058c427354f00 1862 1860 2014-09-04T12:48:43Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 91aeebb2348f629e5b02e751d062e5f5f0f12ac6 1864 1862 2014-09-04T14:52:48Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="3"|'''Tuesday, 9 September 2014''' |"Lindego" lecture hall, third floor, right |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 9a95ba88103f3476d5bd08499c6d6cdd108f287b 1865 1864 2014-09-04T14:53:15Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 9d40dbf5c1c336191ae7e511a847a60ed5307322 1866 1865 2014-09-04T14:55:14Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 14591310ce07a11a68302ef967c540a1d8566d8e 1875 1866 2014-09-05T14:01:04Z Gsawgwikiadmin 1 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:10 |---- |10:00 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:15 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:15 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 0d57f25ebf1326aebc80b866dd69ef8b3db3792a 1876 1875 2014-09-05T20:03:41Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:10 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:30 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |10:45 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} c2a22db8f5525b7cf532f00e1bf148f26125fc70 1877 1876 2014-09-05T20:14:26Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 9494063f777eac40e4ee6911bab85d97355a09c3 1878 1877 2014-09-07T19:22:03Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9 Gaia Data Archive |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} ebd713d3112382a21efd4c705dd9230ccc240700 1880 1878 2014-09-08T10:59:06Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:05 |---- |13:35 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:05 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:35 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:00 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:30 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |17:00 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:25 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:45 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:30 |---- |12:15 | |''Discussion'' |0:45 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 3933265cf61264584ca5dbae265b7c2eb9ef5da0 1882 1880 2014-09-09T12:31:16Z Lukasz 2 wikitext text/x-wiki Draft agenda, subject to changes. '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:30 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 764968cc82f03ebb07a8c10e01738fa259cdf747 1885 1882 2014-09-09T15:29:54Z Lukasz 2 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:30 |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 5c22486f7634c2a79d5ef2d35c9743ae43fe5b35 1889 1885 2014-09-10T12:06:05Z Lukasz 2 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 | |'''Workshop photo''' | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} acb3a998543c1b3fc4c691b9e83eda1dd92441c5 1890 1889 2014-09-11T07:28:11Z Lukasz 2 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 | |'''Workshop photo''' [[Media:workshopphoto2014.jpg]] | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 31d42382820e4d9ab00ce27f6ad721edf7a51392 1892 1890 2014-09-11T07:29:23Z Lukasz 2 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 | |[[Media:workshopphoto2014.jpg |Workshop photo]] | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Zsolt Paragi (JIVE) |Tidal Disruption Events and the search for Massive Black Holes (<10^6 Msun) |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |16:35 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:55 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |17:20 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} be15fa5a72b9dc8d9e4c95513f1a9ded4aa8a761 1895 1892 2014-09-11T12:04:19Z Lukasz 2 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Zbigniew Kołaczkowski (Wrocław) |Wroclaw Observatory |0:15 |---- |13:00 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:15 |Yogesh Joshi (ARIES) |Multi-domian analysis in the Nainital Microlensing Survey data |0:15 |---- |13:30 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 91da59ad1e8120f1cd492a09557f3bdd24aee3a6 1896 1895 2014-09-11T20:20:53Z Lukasz 2 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 339800ce6827f6297716c87d96972547024ec68f 1899 1896 2014-09-20T17:14:52Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} da59c8f841b8ff1af2e29ea7844c2ed3f14d34a5 1900 1899 2014-09-20T17:15:47Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 398b37bf5f38528928800ea14247aed28bccb6ad 1901 1900 2014-09-20T17:16:57Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |OGLE-IV overview |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 6039a2fdb35df5a67d43531d3f9a3a9251cf3c66 6 240 1854 2014-09-02T19:01:40Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1861 1854 2014-09-03T15:13:18Z Gsawgwikiadmin 1 uploaded a new version of &quot;[[File:AbstractBook2014.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1863 1861 2014-09-04T12:50:41Z Gsawgwikiadmin 1 uploaded a new version of &quot;[[File:AbstractBook2014.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1879 1863 2014-09-08T09:23:36Z Lukasz 2 uploaded a new version of &quot;[[File:AbstractBook2014.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 1881 1879 2014-09-08T11:03:15Z Lukasz 2 uploaded a new version of &quot;[[File:AbstractBook2014.pdf]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 233 1855 1850 2014-09-03T06:25:36Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Kester Smith, MPIA Heidelberg, Germany #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL #John Davies, Edinburgh, UK #Igor Soszynski, OAUW, Poland #Johanna Jarvis, Open University, UK 54d5c60d60ab41f4fdacb243071289cc95c1440d 1857 1855 2014-09-03T07:45:31Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> *If you still feel like joining us, please email us asap at gaiasciencealertsworkshop2014 at gmail.com! <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL #John Davies, Edinburgh, UK #Igor Soszynski, OAUW, Poland #Johanna Jarvis, Open University, UK 828f48f2e1d2ee5052e4b240b7053a81ad8fc39e 1883 1857 2014-09-09T14:30:46Z Lukasz 2 wikitext text/x-wiki <big>'''The registration is now closed*!'''</big> <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL #John Davies, Edinburgh, UK #Igor Soszynski, OAUW, Poland #Johanna Jarvis, Open University, UK f20357e8bf5bed60cb1e698fe0a35d66ef91d236 1884 1883 2014-09-09T14:30:53Z Lukasz 2 wikitext text/x-wiki <!--[[Workshop2014:registrationform|Please fill the registration form here]] by '''1st August 2014'''. ---> ===== List of registered participants: ===== #Weronika Narloch, CAMK, Warsaw, Poland #Yogesh Chandra Joshi, ARIES, India #Liam Hardy, University of Sheffield, UK #Krystian Ilkiewicz, OAUW, Poland #Nadejda Blagorodnova, IoA, Cambridge, UK #Andrzej Pigulski, IAUWr, Wroclaw, Poland #Peter Jonker, SRON, Netherlands #Adam Miller, JPL/Caltech, USA #Thomas Wevers, RU Nijmegen, Netherlands #Hasan H. Esenoglu, TUBITAK, Turkey #Heather Campbell, IoA, Cambridge, UK #Milan Stojanovic, AO Belgrade, Serbia #Jochen Greiner, MPG, Garching, Germany #Simon Hodgkin, IoA, Cambridge, UK #Sjoert van Velzen, Nijmegen, Netherlands #Zsolt Paragi, JIVE, Netherlands #Orhan Erece, Akdeniz University, Turkey #Michel Dennefeld, IAP, France #Morgan Fraser, IoA, Cambridge, UK #Patricia Whitelock, SAAO, South Africa #Timo Prusti, ESA, Netherlands #Nami Mowlawi, University of Geneva, Switzerland #Giuseppe Altavilla, INAF-Astronomical Observatory of Bologna, Italy #Jan Soldan, SBIG, Czech Republic #Francois Taris, Paris Observatory, France #Martin Dominik, St.Andrews, UK #Lovro Palaversa, Geneva Observatory, Switzerland #Klaudia Kowalczyk, CAMK, Warsaw, Poland #Chris Davis, Liverpool, UK #Iain Steele, Liverpool, UK #Jure Japelj, Ljubljana, Slovenia #Susanna D. Vergani, CNRS, France #Andrzej Piascik, Liverpool, UK #Werner Zeilinger, Vienna, Austria #Wyn Evans, IoA, Cambridge, UK #Robert Barnsley, Liverpool, UK #Krzysztof Hryniewicz, Geneva, Switzerland #Gerry Gilmore, IoA, Cambridge, UK #Elme Breedt, Warwick, UK #Dan Maoz, Tel-Aviv, Israel #Marcin Semczuk, OAUW, Poland #Krzysztof Ulaczyk, OAUW, Poland #Seppo Mattila, Turku, Finland #Michal Pawlak, OAUW, Poland #George Seabroke, MSSL, UK #Massimo Turatto, Padova, Italy #Zbigniew Kolaczkowski, Wroclaw, Poland #Anna Hourihane, IoA, Cambridge, UK #Malgorzata van Leeuwen, IoA, Cambridge, UK #Cosimo Inserra, QUB, Belfast, UK #Barbara Handzlik, OAUW, Poland #Guy Rixon, IoA, Cambridge #Lukasz Wyrzykowski, OAUW, Poland #Szymon Kozlowski, OAUW, Poland #Zuzanna Kostrzewa-Rutkowska, OAUW, Poland #Alicja Rynkiewicz, OAUW, Poland #Monika Sitek, OAUW, Poland #Krzysztof Rybicki, OAUW, Poland #Dorota Skowron, OAUW, Poland #Kailash Sahu, STSI, USA #Christine Ducourant, Bordeaux, France #Andrzej Udalski, OAUW, Poland #Anthony Brown, Leiden Observatory, NL #Gráinne Costigan, Leiden Observatory, NL #John Davies, Edinburgh, UK #Igor Soszynski, OAUW, Poland #Johanna Jarvis, Open University, UK 465b383ad8e6bdb0324cdc117130ec2a87efd7c2 0 227 1867 1757 2014-09-04T15:00:04Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Railway Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the main part of the workshop will take place in "Lindego" lecture room (formerly room 316). Note, you have to show your workshop badge to the security by the main entrance. On the 12 September (Friday) the workshop will take place in a smaller room number 256, second floor. [[File:buw-foto.jpg]] [[File:buw-lecture-room|250px| Lindego lecture room entrance]] [[File:buw-sal.jpg|250px| Lindego lecture room ]] [[File:buw-around|250px]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the city centre: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] * [http://www.lazienkowski.pl/ Łazienkowski] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 0e2383e9a455cd694571086db5a3be1c9754f6f4 1868 1867 2014-09-04T15:03:07Z Gsawgwikiadmin 1 /* Workshop venue */ wikitext text/x-wiki =Travel info= == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop venue = [http://www.buw.uw.edu.pl/en/ New Library of the University of Warsaw = Nowa Biblioteka Uniwersytetu Warszawskiego (BUW)] [[File:map.png|600px]] [https://www.google.com/maps/place/Warsaw+University+Library/@52.242647,21.024886,17z/data=!3m1!4b1!4m2!3m1!1s0x471ecc5c6af85285:0x8eb2228ca1bb062a Google Map] The Library is located at 56/66 Dobra Street and can be reached by buses number: 105, 118, 127 (stop: Biblioteka Uniwersytecka). Another option is by reaching the main entrance to the University on Krakowskie Przedmiescie Street (e.g. bus 175, which also goes from/to the Chopin Airport and Central Railway Station) and then walk down via Obozna and Leszczynska street until Dobra Street. The Library is located relatively near to the [http://www.kopernik.org.pl/en/ Copernicus Science Center]. For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Central Railway Station: [http://jakdojade.pl?fn=przyst.+DW.+CENTRALNY&fs=DW.+CENTRALNY&fc=52.2291:21.00295&tn=52%C2%B014'30%22%2C+21%C2%B01'28%22&tc=52.24189:21.02463&d=09.07.14&h=13:00&ia=false&t=1&n=0&ri=0&cid=3000&as=true&apv=subway], or from the Centrum to the University and then walk towards the New Library: [http://jakdojade.pl?fn=52%C2%B013'47%22%2C+21%C2%B00'42%22&fc=52.2298:21.01182&tn=52%C2%B014'22%22%2C+21%C2%B01'18%22&tc=52.2395:21.02187&ia=false&t=1&n=0&ri=0&cid=3000&as=true] On the 9-11 September the main part of the workshop will take place in "Lindego" lecture room (formerly room 316). Note, you have to show your workshop badge to the security by the main entrance. On the 12 September (Friday) the workshop will take place in a smaller room number 256, second floor. [[File:buw-foto.jpg]] [[File:buw-lecture-room.jpg|250px| Lindego lecture room entrance]] [[File:buw-sal.jpg|250px| Lindego lecture room ]] [[File:buw-around.jpg|250px]] = Accommodation = The venue of the workshop is located near the Warsaw centre and near the nice area of the Old Town and the Royal Track (Krakowskie Przedmiescie, Nowy Swiat). Here is the list of hotels in the city centre: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] * [http://www.lazienkowski.pl/ Łazienkowski] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] ee5f742e217d67407dfc7750c761d0e3968d48fc 6 241 1869 2014-09-04T15:03:15Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 242 1870 2014-09-04T15:03:32Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 181 1871 1638 2014-09-04T15:09:01Z Gsawgwikiadmin 1 uploaded a new version of &quot;[[File:ScienceAlerts-timeline.png]]&quot; wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 203 1872 1735 2014-09-04T15:22:28Z Gsawgwikiadmin 1 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercatore ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 56849d6d9ad9049f88c15374c43df3ccbcd90492 1873 1872 2014-09-04T15:55:16Z Gsawgwikiadmin 1 /* Belgian Mercatore */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercator ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 05c77b6dfd843e4e0c81b41b75341682b0760768 1874 1873 2014-09-05T08:48:13Z Gsawgwikiadmin 1 /* Swiss Euler */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercator ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 90c771087044a8bbb1eb2e17ab86933ebbac13dd 0 238 1886 1837 2014-09-09T23:24:31Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat?'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Copperwheat?'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 9fe6da777b0161e4033c18368f1edff9aa9aa63f 1888 1886 2014-09-09T23:59:06Z Sth 6 /* Observing Manual */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat?'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Copperwheat?'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/8/81/Gaia_ground_based_followup.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' ea0b37bf3238888ac3ba320b500960168477b3ee 1898 1888 2014-09-14T04:35:13Z Sth 6 /* Observing Manual */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat?'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Copperwheat?'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 3fb40f7b6714cb631386f40343a560cd5e9f7e7e 6 243 1887 2014-09-09T23:58:11Z Sth 6 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 244 1891 2014-09-11T07:28:26Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 226 1893 1740 2014-09-11T07:30:33Z Lukasz 2 wikitext text/x-wiki == Welcome! == [[File:Poster2014.jpg|right|300px|Poster]] '''The fifth Gaia Science Alerts workshop will be held in [[Workshop2014:logistics | Warsaw on 9-12 September 2014]].''' The topics this year include: * Status of Gaia * First Alerts and preliminary results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy The last day (Friday 12th) will be reserved for smaller focused groups meetings. ---- * [[workshop2014:rationale|Rationale]] * [[workshop2014:agenda|Agenda]] * [[workshop2014:registration|Participants and Registration]] * [[workshop2014:logistics|Logistic information]] * [[workshop2014:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Simon Hodgkin * Gerry Gilmore * Nic Walton * Szymon Kozlowski * Heather Campbell * Morgan Fraser * Nadejda Blagorodnova LOC: * Zuzanna Kostrzewa-Rutkowska * Alicja Rynkiewicz * Lukasz Wyrzykowski * Szymon Kozlowski * Krzysztof Rybicki * Monika Sitek ---- Workshop photo (by K.Ulaczyk) [[File:workshopphoto.jpg|300px]] 8b30f9058ff736e837578efbe1be0ceba1eb6e41 6 245 1894 2014-09-11T07:31:01Z Lukasz 2 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 246 1897 2014-09-14T04:34:42Z Sth 6 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 231 1902 1901 2014-09-20T17:18:50Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 22fc86a583086aac0417affe047f98671a7b9849 1903 1902 2014-09-20T17:21:02Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} e1f2ad61226b84f69cf4275078dbfd7df815a904 1904 1903 2014-09-20T17:23:39Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 95d985e2ab7e06811d9345699f99da69f78d3a43 1905 1904 2014-09-20T17:24:56Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} d83a4134d30a95320fa1defab9deaa7bc877f766 1906 1905 2014-09-20T17:28:41Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} df60eed882439b352131c79fac7dfbfc53d6fd82 1907 1906 2014-09-20T17:32:13Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 6fda91b0fa033f89d2f8ea247a872d69065596c7 1908 1907 2014-09-20T17:35:06Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 55e0df3c34ed5c3dc254e9042a97d581bd018201 1909 1908 2014-09-29T15:05:26Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/videos/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 8b6a2dbce15c430add17f906fe3e2d3635a9c0cf 1910 1909 2014-09-29T15:07:32Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.pdf pdf] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.pdf pdf] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.pdf pdf] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.pdf pdf] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.pdf pdf] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.pdf pdf] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.pdf pdf] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.pdf pdf] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.pdf pdf] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.pdf pdf] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.pdf pdf] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.pdf pdf] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.pdf pdf] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.pdf pdf] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.pdf pdf] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.pdf pdf] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.pdf pdf] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.pdf pdf] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.pdf pdf] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.pdf pdf] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.pdf pdf] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.pdf pdf] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.pdf pdf] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.pdf pdf] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.pdf pdf] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.pdf pdf] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.pdf pdf] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.pdf pdf] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.pdf pdf] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.pdf pdf] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.pdf pdf] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.pdf pdf] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.pdf pdf] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.pdf pdf] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.pdf pdf] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.pdf pdf] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.pdf pdf] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.pdf pdf] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.pdf pdf] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.pdf pdf] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.pdf pdf] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.pdf pdf] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.pdf pdf] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 87adb1d90917f2e8f16b5b0d94fe2ae54f162abc 1911 1910 2014-09-29T15:10:50Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 43f5b907d1e3bddd4c01be77d5e946744ee6122b 1912 1911 2014-09-29T15:11:32Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf | menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 7adbd8131863a41d545d571537487c8043494834 1913 1912 2014-09-29T15:13:32Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf |menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 6ecb0f5397e2d65ae187718df3ab9012527dfc04 1914 1913 2014-09-29T15:14:39Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf |menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 792a39b2bf6a6f7ccfb28363f4e32772e36a26fd 1915 1914 2014-09-29T15:15:19Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf |menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf][http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 5f9406a7a014434e0a3f48098428478871279624 1916 1915 2014-09-29T15:17:02Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf |menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDenefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 13f910fb7910da1b010a8eabdb2a7e1b75fdaaf4 1919 1916 2014-10-06T08:05:53Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf |menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZellinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDennefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 728995676019fd0a8f5bfdd07831b7367d0fcd15 1920 1919 2014-10-06T08:06:55Z Zuzanna 36 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2014.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 9 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |10:00 |'''registration desk open''' |(by the main entrance) | |---- |12:00 |'''lunch''' | |1:30 |---- |13:30 | |Welcome |0:15 |---- |13:45 |Timo Prusti (ESA) |Gaia overview and status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/TimoPrusti.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/TimoPrusti.mov rec] |0:30 |---- |14:15 |Anthony Brown (Leiden) |Gaia data processing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnthonyBrown.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnthonyBrown.mov rec] |0:30 |---- |14:45 |Simon Hodgkin (Cambridge) |Gaia Science Alerts Operations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin.mov rec] |0:25 |---- |15:10 |Łukasz Wyrzykowski (Warsaw) |Design of AlertPipe [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski.mov rec] |0:30 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |Guy Rixon (Cambridge) |Technical challenges and solutions for Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GuyRixon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GuyRixon.mov rec] |0:30 |---- |16:40 |George Seabroke (MSSL) |Gaia Radial Velocity Spectrometer follow-up of Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GeorgeSeabroke.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GeorgeSeabroke.mov rec] |0:25 |---- |17:05 |Nami Mowlawi (Geneva) |CU7 variability processing and analysis [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NamiMowlavi.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NamiMowlavi.mov rec] |0:25 |---- |17:30 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 10 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Christine Ducourant (Bordeaux) |The millions of tiny galaxies that Gaia is observing [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChristineDucourant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChristineDucourant.mov rec] |0:25 |---- |09:55 |Grainne Costigan (Leiden) |CU9: Design and Implementation of the Gaia Catalogue [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/GrainneCostigan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/GrainneCostigan.mov rec] |0:20 |---- |10:15 |Massimo Turatto (Padova) |Asiago supernova programme [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MassimoTuratto.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MassimoTuratto.mov rec] |0:15 |---- |10:30 |Andrzej Piascik (Liverpool) |A Spectrograph for the Rapid Analysis of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejPiascik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejPiascik.mov rec] |0:15 |---- |10:45 |'''coffee''' | |0:35 |---- |11:20 |Nadia Blagorodnova (Cambridge) |Gaia: a Supernova Discovery Machine [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/NadiaBlagorodnova.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/NadiaBlagorodnova.mov rec] |0:30 |---- |11:50 |Morgan Fraser (Cambridge) |Validating Gaia Alerts with ground based spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MorganFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MorganFraser.mov rec] |0:25 |---- |11:15 |Simon Hodgkin (Cambridge) |Spectroscopic follow-up of Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SimonHodgkin2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SimonHodgkin2.mov rec] |0:15 |---- |12:30 | |''Discussion'' |0:25 |---- |12:55 |[[Media:workshopphoto2014.jpg |Workshop photo]] | | |---- |13:00 |'''lunch''' | |1:00 |---- |14:00 |Andrzej Udalski (Warsaw) |OGLE-IV overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AndrzejUdalski.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AndrzejUdalski.mov rec] |0:45 |---- |14:45 |Adam Miller (Caltech) |Current and Future Palomar Time-Domain Surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AdamMiller.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AdamMiller.mov rec] |0:25 |---- |15:10 |Dorota Skowron (Warsaw) |The All-Sky Automated Survey for Super Novae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DorotaSkowron.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DorotaSkowron.mov rec] |0:20 |---- |15:30 |'''coffee''' | |0:30 |---- |16:00 |Cosimo Inserra (Belfast) |Overview of PESSTO [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/CosimoInserra.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/CosimoInserra.mov rec] |0:30 |---- |16:30 |Heather Campbell (Cambridge) |Type Ia Supernovae - Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HeatherCampbell.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HeatherCampbell.mov rec] |0:25 |---- |16:55 |Seppo Mattila (Turku) |Supernovae in nuclear environments [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SeppoMattila.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SeppoMattila.mov rec] |0:25 |---- |17:20 |'''end of day 2''' | | |---- |18:00 |'''optional exhibition [http://www.zacheta.art.pl/en/article/view/2002/kosmos-wzywa-sztuka-i-nauka-w-dlugich-latach-szescdziesiatych Cosmos calling!]''' |''price: 10 PLN per person'' | |---- |19:30 |'''workshop dinner''' |'''Zacheta Art Gallery and Restaurant''' ([[Media:dinnermenu.pdf |menu]]) ''price: 190 PLN per person'' | |---- | | | | |---- |colspan="4"|'''Thursday, 11 September 2014''' '''("Lindego" lecture hall, third floor, right)''' |---- |09:30 |Elme Breedt (Warwick) |Accreting compact objects in the transient sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ElmeBreedt.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ElmeBreedt.mov rec] |0:25 |---- |09:55 |Peter Jonker (SRON) |The Gaia Science Alerts potential for discovering intermediate-mass black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/PeterJonker.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/PeterJonker.mov rec] |0:25 |---- |10:20 |Thomas Wevers (Nijmegen) |Probing a new region of phase-space: very short timescale variability with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ThomasWevers.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ThomasWevers.mov rec] |0:25 |---- |10:45 |'''coffee''' | |0:45 |---- |11:30 |Jure Japelj (Ljubljana) |Hunting for GRB afterglows with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JureJapelj.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JureJapelj.mov rec] |0:25 |---- |11:55 |Dan Maoz (Tel Aviv) |Fast Radio Bursts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/DanMaoz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/DanMaoz.mov rec] |0:25 |---- |12:20 |Wyn Evans (Cambridge) |Predicting Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WynEvans.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WynEvans.mov rec] |0:25 |---- |12:55 |'''lunch''' | |1:05 |---- |14:00 |Martin Dominik (St.Andrews) |Measuring masses - Microlensing with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MartinDominik.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MartinDominik.mov rec] |0:25 |---- |14:25 |Kailash Sahu (STSI) |Astrometric Microlensing with GAIA [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KailashSahu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KailashSahu.mov rec] |0:25 |---- |14:50 |Sjoert van Velzen (Nijmegen) |Optical TDE and Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/SjoertvanVelzen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/SjoertvanVelzen.mov rec] |0:25 |---- |15:15 |Krzysztof Hryniewicz (Geneva) |Search for TDE candidates with Swift BAT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofHryniewicz.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofHryniewicz.mov rec] |0:25 |---- |15:40 |'''coffee''' | |0:30 |---- |16:10 |John Davies (Edinburgh) |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohnDavies.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohnDavies.mov rec] |0:20 |---- |16:30 |Anna Hourihane (Cambridge) |Gaia outreach in the UK [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/AnnaHourihane.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/AnnaHourihane.mov rec] |0:25 |---- |16:55 |'''end of day 3''' | | |---- |'''19:00''' |'''Gerry Gilmore (Cambridge)''' |'''Public Talk in the [http://www.kopernik.org.pl/en/ Copernicus Science Centre]''' ''(ticketed,free for workshop attendees)'' | |---- | | | |---- |colspan="3"|'''Friday 12 September 2014''' '''(lecture room 256, second floor, left)''' |'''''NOTE CHANGE OF ROOM''''' |---- |09:30 |Łukasz Wyrzykowski (Warsaw) |Time-domain Network within OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LukaszWyrzykowski2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LukaszWyrzykowski2.mov rec] |0:20 |---- |09:50 |Krzysztof Ulaczyk (Warsaw) |Ephemeris tools for follow-up planning [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/KrzysztofUlaczyk.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/KrzysztofUlaczyk.mov rec] |0:05 |---- |09:55 |Liam Hardy (Sheffield) |pt5m on La Palma - ready to follow up Gaia transients [http://prezi.com/i8irmpyjuail/?utm_campaign=share&utm_medium=copy&rc=ex0share] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LiamHardy.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LiamHardy.mov rec] |0:15 |---- |10:10 |Jochen Greiner (Garching) |GROND capabilities for Gaia transient follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JochenGreiner.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JochenGreiner.mov rec] |0:15 |---- |10:25 |Hasan Esenoglu (Tubitak) |Photometric Contribution to Gaia Alerts from Robotic and Remote Control TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/HasanEsenoglu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/HasanEsenoglu.mov rec] |0:20 |---- |10:45 |Milan Stojanovic (Belgrade) |Serbian-Bulgarian mini-network telescopes as a part of Gaia-Follow-Up Network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MilanStojanovic.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MilanStojanovic.mov rec] |0:15 |---- |11:00 |'''coffee''' | |0:30 |---- |11:30 |Chris Davis (Liverpool) |Time domain astronomy with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/ChrisDavis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/ChrisDavis.mov rec] |0:15 |---- |11:45 |Werner Zeilinger (Vienna) |Gaia Science Alerts: Report on test observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/WernerZellinger.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/WernerZeilinger.mov rec] |0:15 |---- |12:00 |Michel Dennefeld (Paris) |Joint observations for Gaia alerts at OHP [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichelDenefeld.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichelDennefeld.mov rec] |0:15 |---- |12:15 |Lovro Palaversa (Geneva) |Geneva Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/LovroPalaversa.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/LovroPalaversa.mov rec] |0:15 |---- |12:30 |Johanna Jarvis (Open University) |PIRATE's on board [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/JohannaJarvis.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/JohannaJarvis.mov rec] |0:15 |---- |12:45 |Michał Pawlak (Warsaw) |Warsaw Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/slides/MichalPawlak.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2014/movies/MichalPawlak.mov rec] |0:15 |---- |13:00 |'''lunch''' | | |---- | |'''end of day 4''' | | |---- |} 04275c8498cf25bd696ccbf00128173a94cdbbcc 0 238 1917 1898 2014-09-30T11:13:12Z Sth 6 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Jonker'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 8b3bbc24554e642965c7fbb35b0642185c777f13 1929 1917 2014-10-23T08:59:45Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 0cdaeda1129f50ff79e3e020d6beae32b7eb49ee 1933 1929 2014-11-06T12:32:14Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || "Hodgkin, Campbell" |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || "Campbell" |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 880b7ac41b68872488f103e69b13c8f06d793cd1 1934 1933 2014-11-06T12:32:46Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' a807a87fec2e6786f1ac8c9bb999b204f7b444cc 1935 1934 2014-11-10T13:49:36Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Blagorodnova, Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' bde278cba0cc9aaa9170f07eeb8deb3492f87337 1938 1935 2014-11-17T16:52:24Z Sth 6 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ''Elme'' |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' 4dd771ab39dd6d0abecf1773bc1e7f8d012bc0d9 1944 1938 2015-01-13T16:14:21Z Heather.campbell 37 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ''Elme'' | | 28 Feb, 1 Mar || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ' |- | 7, 8, 9 Feb || 3 || Campbell || ITP2 || INT || IDS || |- | 2-7 May || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' a562fa6850e10138ff8bb89d2d0ea4a889663ff6 1945 1944 2015-01-13T16:14:50Z Heather.campbell 37 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ''Elme'' | | 28 Feb, 1 Mar || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 7, 8, 9 Feb || 3 || Campbell || ITP2 || INT || IDS || |- | 2-7 May || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' ddc2b96f3be39aa82842c8dfd3f890301902122f 1946 1945 2015-01-13T16:15:24Z Heather.campbell 37 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ''Elme'' |- | 28 Feb, 1 Mar || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || |- | 7, 8, 9 Feb || 3 || Campbell || ITP2 || INT || IDS || |- | 2-7 May || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' e7465688842b883dfea354200439d7cc42f594d7 1947 1946 2015-01-23T13:21:29Z Heather.campbell 37 /* Observing Rota */ wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ''Elme'' |- | 28 Feb, 1 Mar || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Fraser'' |- | 7, 8, 9 Feb || 3 || Campbell || ITP2 || INT || IDS || ''Campbell'' |- | 2-7 May || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' b22c612cce9001bdaf3bdc2fbbf157218ac811bc 0 214 1918 1732 2014-09-30T21:21:52Z Sth 6 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #'''Nic Walton [O]''' #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #'''Elme Breedt [O]''' #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #Eran Ofek #Rachel Street #'''Lukasz Wyrzykowski''' #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #Aleks Scholz [O] #Zbigniew Kolaczkowski #'''Chris Davis [O]''' #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #'''Sjoert van Velzen''' [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi === GSAWG6: GRBs === #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Andreja Gomboc #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet 69e94fc36a6106d9df538ec9db72735c0864a8f6 1921 1918 2014-10-09T10:30:11Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj 085869c5486e3e4de3c899769edacb72f9b9f192 1922 1921 2014-10-13T18:52:37Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Horvath Istvan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj a579b749bcee403e4adae9cd3ada2afefd9d88be 1923 1922 2014-10-13T18:53:36Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Horvath Istvan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis e5b8a3c18d1aa520eaab925f73b2295ca8a0ac9d 1924 1923 2014-10-13T18:57:33Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Horvath Istvan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] 29b0988626b3c7cac3d46c29f75c65d36d601b6c 1925 1924 2014-10-14T11:13:24Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Horvath Istvan === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] 8c5d5c2e28407d0a8fa4fc2d3f39819e40841a7a 1926 1925 2014-10-14T13:50:24Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] bd5c34e3f68204b8b6be2f6e92484350e8274896 1927 1926 2014-10-14T13:55:37Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] d9b84b3b149716d9ea7c34c65e0068a9772b6e88 1928 1927 2014-10-16T09:04:16Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik === GSAWG10: Photometric Follow-Up === #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] cc12b37781b353d02744f86823c86b7a26d95ab3 1930 1928 2014-10-27T13:57:13Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] 97c0fe5219dda7efb5f8632e80532067b8680813 1936 1930 2014-11-12T13:52:25Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] 62753b731fe9883f822c4044fd3a1374c326de4c 1937 1936 2014-11-13T09:43:06Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana e063f8e315c69ae43899a9434f396932f9399a54 1939 1937 2014-11-20T10:12:08Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana 73c0b24cf95aa3009f6c6966a7aa351c0c2cec1e 1940 1939 2014-11-25T11:48:56Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana e4ad14e3241da020f13bd3f3a167d217d3afe658 1941 1940 2014-11-25T21:06:34Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana d806660eb70df255479940a544d8a41d1a0a784a 1943 1941 2014-12-11T11:21:32Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana eacc2f3802aa9ae63a15f0c7dd5e7ec3e7eea6b9 1948 1943 2015-01-29T21:06:25Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana 60c78d1288a17455fd09db74e0faed8290ecfc29 1949 1948 2015-01-29T21:10:18Z Lukasz 2 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec 98a54bcb2678a327a0eb5fb7403538eebea34d6c 0 203 1931 1874 2014-10-30T09:46:07Z Lukasz 2 /* Partners in test */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercator ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Vega Slovenia ==== * Contact person: Jure Japelj * Location: Ljubljana, Slovenia * 0.7m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 4de3ae4e926e443b014a201472c39dee672d6862 1932 1931 2014-10-30T09:46:46Z Lukasz 2 /* Swiss Euler */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercator ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Vega Slovenia ==== * Contact person: Jure Japelj * Location: Ljubljana, Slovenia * 0.7m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> 1138ddbaefa6d1565ba23b85032aaa0dc38f7cbe 1942 1932 2014-11-29T13:21:00Z Lukasz 2 /* Tubitak Turkey */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercator ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1,3 ), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Vega Slovenia ==== * Contact person: Jure Japelj * Location: Ljubljana, Slovenia * 0.7m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> cd87afeaf0403256954543633424bda4db11655b 0 17 1950 1761 2015-02-05T16:20:01Z Arancha.delgado 39 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == 0ed9ce4f519799b32033f50f08ab0ab32a422709 1951 1950 2015-02-05T16:24:06Z Arancha.delgado 39 /* GAIA Marshall */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. == Catalogues Cross-matched and Update Frequencies == * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours dcfa1adb9c826b425332fca80e6f86094900881e 0 17 1952 1951 2015-02-05T16:25:36Z Arancha.delgado 39 /* Catalogues Cross-matched and Update Frequencies */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. == Catalogues Cross-matched and Update Frequencies == * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour 4022feb5291098b506998501bab1247c8ae5d730 1953 1952 2015-02-05T16:25:56Z Arancha.delgado 39 /* Catalogues Cross-matched and Update Frequencies */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. === Catalogues Cross-matched and Update Frequencies === * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour 8bd797e6d569a77f388ec8201ef48013e370b7fc 1954 1953 2015-02-05T16:26:37Z Arancha.delgado 39 /* Catalogues Cross-matched and Update Frequencies */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. ==== Catalogues Cross-matched and Update Frequencies ==== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour b98612e4d09a8b5c48e0f8677d2a7d3fb438d388 1955 1954 2015-02-05T16:27:02Z Arancha.delgado 39 /* Catalogues Cross-matched and Update Frequencies */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour 92b8401a7ecb39a032e3c02744becc1b3ede4c6b 1956 1955 2015-02-05T16:35:06Z Arancha.delgado 39 /* Catalogues Cross-matched and Update Frequencies */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====Other ===== * Gaia Marshall how-to * Tutorial * Known bugs * Tracking Modifications 92bf643c9f78daa83a6329ed7517641864e546ff 1957 1956 2015-02-05T16:35:55Z Arancha.delgado 39 /* Other */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * Gaia Marshall how-to * Tutorial * Known bugs * Tracking Modifications 10e258074d184a40bd256f9063f6222379710bf7 1958 1957 2015-02-05T17:06:05Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * Gaia Marshall how-to * Tutorial * Known bugs * Tracking Modifications 501852960d0ffd6475ce7cdf54d9656db0f3f05c 1959 1958 2015-02-06T12:30:24Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * Gaia Marshall how-to [[marshall how-to]] * Tutorial * Known bugs 9c57a7d2ea22731b6477e841555cf97d24daf8b9 1964 1959 2015-02-06T12:39:03Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * Gaia Marshall how-to: [[marshall how-to]] * Tutorial: [[File:gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 5080bb522fc14ffdf8cd9c05fef496021b624bca 1967 1964 2015-02-06T12:43:07Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * [[Gaia Marshall how-to]] * Tutorial: [[File:gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 9bacb97ad7f3570f65bd742d7464e7c4aae57bb7 1969 1967 2015-02-06T12:48:59Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * [[Gaia Marshall how-to]] * Tutorial: [[media:gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 1d152e097228eb5eb0acb2b14d4f9ff6dc144e10 1970 1969 2015-02-06T12:49:32Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * [[Gaia Marshall how-to]] * Tutorial: [[gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] cb66acd9c2856e2210e48707eb9a494421b85359 1971 1970 2015-02-06T12:52:07Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * [[marshall how-to]] * Tutorial: [[gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 46a88b1db1a2f6a3aba8243b4a9a98b72c1a489b 1972 1971 2015-02-06T12:54:03Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====More Info ===== * [[marshall how-to]] * [[File: Gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 21f7e13878636f5818c91f926515968161187608 1973 1972 2015-02-06T12:54:48Z Arancha.delgado 39 /* More Info */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====Marshall how-tos and Known bugs===== * [[marshall how-to]] * [[File: Gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 42c2e605a833210cfadffeb5e1bf96fdf37f3a76 1974 1973 2015-02-06T12:55:13Z Arancha.delgado 39 /* Marshall how-tos and Known bugs */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * LSQ: ** New discoveries: Every 30 min ** Recalibrated: Every 1 hour * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====Marshall How-to and Known Bugs===== * [[marshall how-to]] * [[File: Gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 6941ae40c21094f80bee01195864bf866915f06c 1998 1974 2015-06-24T09:14:52Z Arancha.delgado 39 /* GAIA Marshall */ wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by SkyAlert.org. <big> Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====Marshall How-to and Known Bugs===== * [[marshall how-to]] * [[File: Gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] fa49f37ecd1f3442df0af5c32f8bb4a456a6bac5 0 247 1960 2015-02-06T12:32:41Z Arancha.delgado 39 Created page with "==GAIA Marshall How-to== # All the new GAIA Alerts are collected in the "Inbox". # If you decide that a GAIA source is worth to classify, select the action "Classification targe..." wikitext text/x-wiki ==GAIA Marshall How-to== # All the new GAIA Alerts are collected in the "Inbox". # If you decide that a GAIA source is worth to classify, select the action "Classification targets" and the object will be moved from the "Inbox" to "Classification targets" inbox. # Once the source is already in "Classification Targets" if there is already a good spectrum of the source, select "Classify" action. A form with several input fields will show up in your screen for fulfilling with the details of the object. When you submit this form the alert will be moved to "Classified" and to "Review to Followup" inboxes. If in the classification form you also ticked the checkbox for Atel submission, the object will also appear in "Queued for Atel". # If the source is in "Classification Targets" and there is not an spectrum of it, select the action "Observed" and the source will be moved to "Queued for Classification". After observing the object: *** If you get a good quality spectrum, select the action "Classify". *** If the spectrum quality is not good enough, you can send it back to "Classification Targets" inbox selecting the action "Classification targets". # If the source looks very interesting you might want to take on further observations. From "Review to followup" you can send the object to "Followup Targets" choosing the action "Followup Targets". # Either from "Queued for Atel", "Classified" or "Followup targets" you can conclude the followup selecting the action "Followup Complete". The object will be moved to "Followup Complete" inbox. # From all inboxes you can decide that the object is not worth to investigate and send it to "All Archived". # The sources from the other catalogues (CRTS, ASAS, OGLE, etc.) will go directly to "External Sources Inbox" (not shown in the this diagram), and are only used for cross-matching purposes. f08f97befcd3b3442d592ba9fff9cccf1a18476f 1961 1960 2015-02-06T12:33:17Z Arancha.delgado 39 /* GAIA Marshall How-to */ wikitext text/x-wiki ==GAIA Marshall How-to== # All the new GAIA Alerts are collected in the "Inbox". # If you decide that a GAIA source is worth to classify, select the action "Classification targets" and the object will be moved from the "Inbox" to "Classification targets" inbox. # Once the source is already in "Classification Targets" if there is already a good spectrum of the source, select "Classify" action. A form with several input fields will show up in your screen for fulfilling with the details of the object. When you submit this form the alert will be moved to "Classified" and to "Review to Followup" inboxes. If in the classification form you also ticked the checkbox for Atel submission, the object will also appear in "Queued for Atel". # If the source is in "Classification Targets" and there is not an spectrum of it, select the action "Observed" and the source will be moved to "Queued for Classification". After observing the object: ## If you get a good quality spectrum, select the action "Classify". ## If the spectrum quality is not good enough, you can send it back to "Classification Targets" inbox selecting the action "Classification targets". # If the source looks very interesting you might want to take on further observations. From "Review to followup" you can send the object to "Followup Targets" choosing the action "Followup Targets". # Either from "Queued for Atel", "Classified" or "Followup targets" you can conclude the followup selecting the action "Followup Complete". The object will be moved to "Followup Complete" inbox. # From all inboxes you can decide that the object is not worth to investigate and send it to "All Archived". # The sources from the other catalogues (CRTS, ASAS, OGLE, etc.) will go directly to "External Sources Inbox" (not shown in the this diagram), and are only used for cross-matching purposes. 98a4de4fe7b1d123c54d05bc799a7ae6e67d8228 1963 1961 2015-02-06T12:36:56Z Arancha.delgado 39 /* GAIA Marshall How-to */ wikitext text/x-wiki ==GAIA Marshall How-to== # All the new GAIA Alerts are collected in the "Inbox". # If you decide that a GAIA source is worth to classify, select the action "Classification targets" and the object will be moved from the "Inbox" to "Classification targets" inbox. # Once the source is already in "Classification Targets" if there is already a good spectrum of the source, select "Classify" action. A form with several input fields will show up in your screen for fulfilling with the details of the object. When you submit this form the alert will be moved to "Classified" and to "Review to Followup" inboxes. If in the classification form you also ticked the checkbox for Atel submission, the object will also appear in "Queued for Atel". # If the source is in "Classification Targets" and there is not an spectrum of it, select the action "Observed" and the source will be moved to "Queued for Classification". After observing the object: ## If you get a good quality spectrum, select the action "Classify". ## If the spectrum quality is not good enough, you can send it back to "Classification Targets" inbox selecting the action "Classification targets". # If the source looks very interesting you might want to take on further observations. From "Review to followup" you can send the object to "Followup Targets" choosing the action "Followup Targets". # Either from "Queued for Atel", "Classified" or "Followup targets" you can conclude the followup selecting the action "Followup Complete". The object will be moved to "Followup Complete" inbox. # From all inboxes you can decide that the object is not worth to investigate and send it to "All Archived". # The sources from the other catalogues (CRTS, ASAS, OGLE, etc.) will go directly to "External Sources Inbox" (not shown in the this diagram), and are only used for cross-matching purposes. [[File:Workflow.png]] b201419305cf27b04b8ebf4d19160c6b620e5a10 6 248 1962 2015-02-06T12:36:03Z Arancha.delgado 39 Gaia Marshall data flow wikitext text/x-wiki Gaia Marshall data flow fb93d985815eac6612d05e97368700c9b4e97eaa 0 249 1965 2015-02-06T12:40:50Z Arancha.delgado 39 Created page with "== GAIA Marshall Known Bugs == Please, add any new bug or abnormal functionalities you might find." wikitext text/x-wiki == GAIA Marshall Known Bugs == Please, add any new bug or abnormal functionalities you might find. 624e41ccbf0da8e440749eb5eacd0c913aac1e82 1966 1965 2015-02-06T12:42:12Z Arancha.delgado 39 /* GAIA Marshall Known Bugs */ wikitext text/x-wiki == GAIA Marshall Known Bugs == Please, add any new bug or abnormal functionalities you might find and the date you had the problem. * ... * ... * ... 2ae7bee17d7df3384d7ccb4d279807f125fce9ff 1975 1966 2015-02-06T12:56:20Z Arancha.delgado 39 /* GAIA Marshall Known Bugs */ wikitext text/x-wiki == GAIA Marshall Known Bugs == Please, add any new bug or abnormal functionalities you might find. Don't forget to specify the date you encounter the problem. * ... * ... * ... 33496428de98f4ad3bd4ca7f97bc251757784e89 1977 1975 2015-02-10T13:55:43Z Arancha.delgado 39 /* GAIA Marshall Known Bugs */ wikitext text/x-wiki == GAIA Marshall Known Bugs == Please, add any new bug or abnormal functionalities you might find. Don't forget to specify the date you encounter the problem. * Once an object is classified, this information can not be updated. * ... * ... 034d77ec5ac1eb86411707415bbe5c9e42a0cb05 1983 1977 2015-04-20T13:37:29Z Arancha.delgado 39 /* GAIA Marshall Known Bugs */ wikitext text/x-wiki == GAIA Marshall Known Bugs == Please, add any new bug or abnormal functionalities you might find. Don't forget to specify the date you encounter the problem. * Once an object is classified, this information can not be updated.-> This is fixed now. It is possible to update the classification from every inbox. * ... * ... c84a476870778b3fb50a3455c57ba513f29f8f32 6 250 1968 2015-02-06T12:47:18Z Arancha.delgado 39 Gaia Marshall Tutorial wikitext text/x-wiki Gaia Marshall Tutorial 8c1df14222849e093b59973919e0ee975ba805f0 1978 1968 2015-02-26T14:07:25Z Arancha.delgado 39 uploaded a new version of &quot;[[File:Gaia marshall tutorial.pdf]]&quot; wikitext text/x-wiki Gaia Marshall Tutorial 8c1df14222849e093b59973919e0ee975ba805f0 0 203 1976 1942 2015-02-09T15:38:41Z Gsawgwikiadmin 1 /* NORTH */ wikitext text/x-wiki = Status of the partners preparing for the Gaia Alerts verification = == Information about the requirements == In order to become a member of the Gaia Follow-up Network for Transient Objects (Gaia-FUN-TO), especially to take part in the alerts verification, a potential partner must fullfil a number of requirements. The list of requirements is still to be fine-tuned, but they are: # take part in the test observations # react to an alert (or to a request with a target) and conduct its observations (in multiple filters) within 24h # reduce the photometric data and submit to the [[Follow-up|CPCS]] within 24h from the observation (*) # flux calibrations better than 10% (0.1 mag) (*) ''Note: the CPCS was created in order to facilitate the homogenous calibration of the photometric reductions. You are welcome to provide your own calibrated data and omit the CPCS step, but we will still need to obtain the data within 24h from the observation.'' [[Verification:tests|Test observing campaigns and results]] = Partners in test= === '''NORTH''' === ==== Loiano ==== * Contact person: Gisella Clementini, Giuseppe Altavilla * Location: Loiano, Bologna, Italy * 1.5m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Asiago==== * Contact person: Gisella Clementini, Lina Tomasella * Location: Padova, Italy * 1.82m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== APT2==== * Contact person: Gisella Clementini, Giuseppe Leto, * Location: Serra la Nave, Catania, Sicily * robotic 80cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== TNT ==== * Contact person: Anna Piersimoni * Location: Teramo, Italy, * 72cm Ritchey-Cretien <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Belgian Mercator ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Palma (Swiss time) * 1.2m <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Konkoly==== * Contact person: Laszlo Szabados, Gabor Marschalko * Location: Piszkesteto Mountain Station of the Konkoly Obs., Hungary * 1m RCC, 60/90/180 cm Schmidt, 50 cm Cassegrain <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====PIRATE==== * Contact person: Ulrich Kolb, Richard.Busuttil * Location: Mallorca * 43cm corr.D-K, remote and robotic controlled <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: R. Busuttil, U. Kolb, J. Bochinski (Open University), V. Burwitz (MPE Garching), J. Rodriguez (OAM, Mallorca)'' ==== pt5m ==== * Contact person: Stuart Littlefair * Location: La Palma * 50cm mod.D-K, robotic <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ====Vienna==== * Contact person: Werner Zeilinger * Location: Austria * 1.5m RC <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> Small FoV: occasional problems with calibrations. ====ASV Serbia==== * Contact person: Goran Damljanovic, Oliver Vince * Location: Serbia * 60cm reflector <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ''Names and affiliations: G. Damljanovic, O. Vince, R. Pavlovic, Z. Cvetkovic, M. Stojanovic (Astronomical Observatory, Belgrade)'' ==== Tubitak Turkey ==== * Contact person: Irek Khamitov * Location: Turkey * 150cm (RTT150), 100cm, 60cm <big>Status: <span style="color:#FFFFFF; background:#0000ff">manual data upload within 24h</span></big> ''Names and affiliations: Khamitov I.M.(1,3 ), Esenoglu H.(1,2), Bikmaev I.F.. (3,4), Zhuchkov R.Ya. (3,4) 1. TÜBİTAK National Observatory, Antalya, Turkey 2. İstanbul University, Istanbul, Turkey 3. Kazan Federal University, Kazan, Russia 4. Academy of Sciences of Tatarstan, Kazan, Russia '' ==== Bialkow/Wroclaw Poland ==== * Contact person: Zbyszek Kolaczkowski * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Italian Supernova Project ==== * Contact person: Simone Leonini * Location: Italy * 53cm <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ''Names and affiliations: S. Leonini, M. Conti, G. Guerrini, P. Rosi, L.M. Tinjaca Ramirez, Montarrenti Observatory, Siena, Italy part of Italian Supernovae Serach Project (ISSP)'' ==== Wise Observatory ==== * Contact person: Yossi Shvarzvald, Dani Maoz * Location: Israel * 1m, 71cm, 45cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== Ostrowik Observatory ==== * Contact person: Lukasz Wyrzykowski, Krzysztof Ulaczyk, Michal Pawlak * Location: Poland * 60cm <big>Status: <span style="color:#FFFFFF; background:#00ff00">automated data upload</span></big> ==== OHP ==== * Contact person: Michel Dennefeld * Location: France * 1.2m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> ==== Vega Slovenia ==== * Contact person: Jure Japelj * Location: Ljubljana, Slovenia * 0.7m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ---- === '''SOUTH''' === ==== Swiss Euler ==== * Contact person: Laurent Eyer, Lovro Palaversa * La Silla, Chile * 1.2m <big>Status: <span style="color:#FFFFFF; background:#5500ff">manual data upload</span></big> ====Danish/Czech Telescope ==== * Contact person: Pavel Koubsky and Uffe Jorgensen * La Silla * 1.54m, remotely controlled by Czechs <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== GROND ==== * Contact person: Jochen Greiner, MPIE * 2.2m La Silla * 7 channels: Optical/NIR: grizJHK <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> Some data collected. ==== SAAO ==== * Contact person: Patricia Whitelock * 1.9m, 1.0m <big>Status: <span style="color:#FFFFFF; background:#ff0000">no data uploaded</span></big> f731aa41a84acf88acc46cd4fb6b11cffd399c47 0 251 1979 2015-03-05T10:32:45Z Gsawgwikiadmin 1 Created page with "'''<big><span style="color:#FF0000">This programme is not yet open to everybody!</span></big>''' =Adopt a Supernova= Gaia now detects 1-4 new transients every day. In this (pil..." wikitext text/x-wiki '''<big><span style="color:#FF0000">This programme is not yet open to everybody!</span></big>''' =Adopt a Supernova= Gaia now detects 1-4 new transients every day. In this (pilot) programme you can pick one (or more!) transients detected by Gaia (supernova or any other) and treat it is a your "pet". This involves simply taking care your object is classified and has enough observations so it can be useful for further studies of supernovae. In particular, supernovae Type Ia, once they have their redshift measured and their light curve sampled enough, can be then modelled and be used for cosmological studies of the expansion of the Universe. == Picking a target == Gaia transients are listed on couple of pages. '''''Note: Some pages require authorisation. Please contact us if need the passwords stating who you are and why would like to join this programme.''''' * [http://gaia.ac.uk/selected-gaia-science-alerts selected-gaia-science-alerts] * [http://gaiamarshall.ast.cam.ac.uk/marshall/index.py Gaia Marshall] [https://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/1/10/Gaia_marshall_tutorial.pdf Marshall Manual] * [http://kohav.astrouw.edu.pl/~wyrzykow/cgi-bin/gaiaalertspublic-followup.html Gaia Alerts light curves with photometric follow-up data] The main selection criterion is that the target is still on-going ''(ok, you can also pick one which is now gone, but then not much apart from modelling and studying the target is possible)''. This [http://www.onlineconversion.com/julian_date.htm Online Julian Date converter] can be helpful to understand the Julian Dates plotted on the light curves. Note various offsets on different plots, e.g. JD-2456000 on Gaia light curves. == Taking care of your target == Your task is to make sure your supernova gets enough follow-up data to be useful for studies of supernovae and cosmology. It means that apart from spectral classification (which for a while is out of this programme), it has a nice light curve in multiple bands. If a SN is young (around max) you probably want it to be observed every 3-5 days, but once it is a bit older, say ~10 days afer max, it is enough to observe it once every 7-10 days. Remember, supernovae get fainter so you have to balance your sampling with available telescopes, e.g. you can not wait with collecting next point when it is reaching ~20 mag, as it will be very hard to observe with most instruments we currently have. ==== Requesting observing ==== If you want your supernova to have a new data point there are various ways: * observe it yourself or ask your colleagues to have it observed (Ostrowik, Loiano) * request observations with the LCOGT network (primarily south) - currently request via LW * request observations via Gaia Science Alerts WG10 for Photometric Follow-up via LW (Gaia-FUN-TO: network of European telescopes, so north only) ==== Reducing the data ==== You want to know what is going on with your supernova and taking an image is not enough, of course. You need your data to be reduced as soon as possible. We are currently establishing an automated or semi-automated data reduction pipeline, but many of you know the procedures already! But careful, supernovae are tricky! Especially those very close to their host galaxy and embedded in the diffuse galaxy light. Ultimately, a difference imaging pipeline would be the best for such purpose, but as a first approximation, a SExtractor or similar tool is good enough. Before executing SExtractor, you usually will need to obtain astrometric solution for your image, I suggest using [http://nova.astrometry.net/ astrometry.net]. ==== Submitting the observations to the Calibration Server ==== Once you have obtained magnitudes of all stars from your image in a given filter, then the data needs to be submitted to the [gsaweb.ast.cam.ac.uk/followup/ Calibration Server] (see manual there). This is designed to provide calibrated magnitudes of your supernova as well as to store all follow-up observations. The procedure of submission can be fully automatised and we hope it will be part of the data reduction pipeline. == Final steps == Once your supernova is gone you should make sure that all available data has been reduced and collected at the Calibration Server. You should be able to extract all the data from the Calib Server (authorisation required) and you should then have a critical look at all the measurements. Some will need to be removed due to their errors or large scatter. The remaining light curve should be analysed with an attempt of modelling it. We will later include the details on how to do it. = Enjoy! And clear skies! = 9cace7a2f2ec1f50659a06ab1845b6761ebc3a49 1980 1979 2015-03-05T10:35:05Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big><span style="color:#FF0000">This programme is not yet open to everybody!</span></big>''' =Adopt a Supernova= Gaia now detects 1-4 new transients every day. In this (pilot) programme you can pick one (or more!) transients detected by Gaia (supernova or any other) and treat it is a your "pet". This involves simply taking care your object is classified and has enough observations so it can be useful for further studies of supernovae. In particular, supernovae Type Ia, once they have their redshift measured and their light curve sampled enough, can be then modelled and be used for cosmological studies of the expansion of the Universe. == Picking a target == Gaia transients are listed on couple of pages. '''''Note: Some pages require authorisation. Please contact us if need the passwords stating who you are and why would like to join this programme.''''' * [http://gaia.ac.uk/selected-gaia-science-alerts selected-gaia-science-alerts] * [http://gaiamarshall.ast.cam.ac.uk/marshall/index.py Gaia Marshall] [https://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/1/10/Gaia_marshall_tutorial.pdf Marshall Manual] * [http://kohav.astrouw.edu.pl/~wyrzykow/cgi-bin/gaiaalertspublic-followup.html Gaia Alerts light curves with photometric follow-up data] The main selection criterion is that the target is still on-going ''(ok, you can also pick one which is now gone, but then not much apart from modelling and studying the target is possible)''. This [http://www.onlineconversion.com/julian_date.htm Online Julian Date converter] can be helpful to understand the Julian Dates plotted on the light curves. Note various offsets on different plots, e.g. JD-2456000 on Gaia light curves. == Taking care of your target == Your task is to make sure your supernova gets enough follow-up data to be useful for studies of supernovae and cosmology. It means that apart from spectral classification (which for a while is out of this programme), it has a nice light curve in multiple bands. If a SN is young (around max) you probably want it to be observed every 3-5 days, but once it is a bit older, say ~10 days afer max, it is enough to observe it once every 7-10 days. Remember, supernovae get fainter so you have to balance your sampling with available telescopes, e.g. you can not wait with collecting next point when it is reaching ~20 mag, as it will be very hard to observe with most instruments we currently have. ==== Requesting observing ==== First, check the visibility of your target using [http://www.astrouw.edu.pl/~kulaczyk/ephem/ this tool] (be careful: when entering coords in degrees remember to add "d" before right-ascension). If you want your supernova to have a new data point: * observe it yourself or ask your colleagues to have it observed (Ostrowik, Loiano) * request observations with the LCOGT network (primarily south) - currently request via LW * request observations via Gaia Science Alerts WG10 for Photometric Follow-up via LW (Gaia-FUN-TO: network of European telescopes, so north only) ==== Reducing the data ==== You want to know what is going on with your supernova and taking an image is not enough, of course. You need your data to be reduced as soon as possible. We are currently establishing an automated or semi-automated data reduction pipeline, but many of you know the procedures already! But careful, supernovae are tricky! Especially those very close to their host galaxy and embedded in the diffuse galaxy light. Ultimately, a difference imaging pipeline would be the best for such purpose, but as a first approximation, a SExtractor or similar tool is good enough. Before executing SExtractor, you usually will need to obtain astrometric solution for your image, I suggest using [http://nova.astrometry.net/ astrometry.net]. ==== Submitting the observations to the Calibration Server ==== Once you have obtained magnitudes of all stars from your image in a given filter, then the data needs to be submitted to the [gsaweb.ast.cam.ac.uk/followup/ Calibration Server] (see manual there). This is designed to provide calibrated magnitudes of your supernova as well as to store all follow-up observations. The procedure of submission can be fully automatised and we hope it will be part of the data reduction pipeline. == Final steps == Once your supernova is gone you should make sure that all available data has been reduced and collected at the Calibration Server. You should be able to extract all the data from the Calib Server (authorisation required) and you should then have a critical look at all the measurements. Some will need to be removed due to their errors or large scatter. The remaining light curve should be analysed with an attempt of modelling it. We will later include the details on how to do it. = Enjoy! And clear skies! = b3386a6f5a1a4c93b101bcbd7717d39e9f2a5ca1 0 214 1981 1949 2015-03-07T20:46:03Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett === GSAWG2: CVs and XRBs === #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec d7c4640e8f4316c58851a687b8edcded32618a53 1982 1981 2015-03-07T20:46:57Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett === GSAWG2: CVs and XRBs === This group has already established their own mailing list. Please contact the chair, Elme, if you want to join it. #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec ec1f7027ec9856d45145dbfd913248ea4d5de84e 0 238 1984 1947 2015-06-15T19:30:01Z Gsawgwikiadmin 1 wikitext text/x-wiki On these pages we summarise and coordinate our '''Photometric''' and '''Spectroscopic''' observing runs for the upcoming semesters. This page will be amended as more follow-up runs are scheduled. ===2014B Observing Time Awarded=== The total amounts of time awarded for each semester (so far) is given below. Note that these come from a variety of proposals and awards, submitted by a number of individuals. While these nights should be seen as in a sense pooled, the coordination of the different programmes will be the responsibility of the individual PI's. {| class="wikitable" style="text-align: right" style="border-width: 3px" ! style="text-align:right;" | Telescope !! 2014B !! 2015A |- |Asiago || 30 n || - |- | ESO NTT || 5 n || 0 n |- |INT || 30 n || 3.5 n |- | LT || 170 h || 70 h |- | Mercator || 7 n || 7 n |- | SAAO || - || - |- |WHT || 15 n || 3.5 n |- |Loiano || 29n || - |} ===Observing Rota=== Note that the UK-led runs can be supported by PATT for a maximum of two observers. The NL-led nights will be coordinated by *** and ***. There is **no** PATT funding available for these funds unless no one from the NL community can participate, in which case funding for one observer may be available (**TBD**). {| class="wikitable" style="text-align: right" style="border-width: 3px" ! Dates !! Nights !! PI !! Program !! Telescope !! Instrument !! Observers |- | 20-21 Jul || 2 || Jonker || N4 || INT || IDS || ''Wevers'' |- | 19-23 Aug || 5 || Hodgkin || || NTT || EFOSC2 || ''Hodgkin'' |- | 21-24 Aug || 1+3 || Wevers/Hodgkin || N7/P14 || INT || IDS || ''Campbell+Wevers'' |- | 3-6 Sep || 4 || Hodgkin || P14 || INT || IDS || ''Hodgkin'' |- | 12-16 Sep || 5 || Hodgkin || P14 || INT || IDS || ''Hodgkin'',''Campbell'' |- |15-18 Sep || 4 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 17-27 Sep || 10 || Clementini || - || Loiano || - || ''Ulaczyk, Pawlak + students (Warsaw)'' |- | 29-30 Sep || 1.5 || Fraser || P29 || WHT || ACAM || ''Fraser'' |- | 13-15 Oct || 2 || Velzen || N15 || WHT || ACAM+ISIS || ''Rixon'' |- | 27-28 Oct || 1+1 || Velzen/Fraser || N15/P29 || WHT || ISIS || ''Torres'' |- | 15-18 Nov || 4 || Wevers || N7 || INT || IDS || ''Wevers'' |- | 27-29 Nov || 3 || Fraser || P29 || WHT || ACAM || ''Blagorodnova'' |- | 2-5 Dec || 4 || Hodgkin || P14 || INT || IDS || ''Copperwheat'' |- | 11-14 Dec || 2+2 || Hodgkin/Wevers || P14/N7 || INT || IDS || ''Wevers'' |- | 20-22 Dec || 2.5 || Fraser || P29 || WHT || ISIS || ''Van Velzen'' |- | 30 Dec-3 Jan || 5 || Wevers || N7 || INT || ISIS || ''Torres'' |- | 3-4 Jan || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Jonker'' |- | 5-7 Jan || 3 || Campbell || ITP2 || INT || IDS || ''Hodgkin'' |- | 11-13 Jan || 1/2+1+1/2 || Velzen/Fraser || N15/P29 || WHT || ISIS + ACAM || ''Hodgkin, Campbell'' |- |15-19 Jan || 5 || Campbell || ITP2 || Mercator || Maia || ''Campbell'' |- | 2-5 Mar || 4 || Campbell || ITP2 || Marcator || Maia || ''Elme'' |- | 28 Feb, 1 Mar || 2 || Campbell || ITP2 || WHT || ISIS+ACAM || ''Fraser'' |- | 7, 8, 9 Feb || 3 || Campbell || ITP2 || INT || IDS || ''Campbell'' |- | 2-7 May || 4 || Campbell || ITP2 || Marcator || Maia || |} === Observing Manual === The Gaia Follow-up observers Manual will be available '''HERE''' http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/6/6f/Fuga-handbook.pdf === Gaia Marshal === The Gaia Follow-up Marshal will be available '''HERE''' === ATel Guidelines === How to prepare your ATel on Gaia Alerts follow-up. [[ATEL Spectra with Gaia | Spectroscopy awarded to people related with GSA ]] [[ATEL Phot no Gaia | Photometric follow-up without Gaia people]] 21c99ec8c28f648b50958dc47e5861743b74292d 0 252 1985 2015-06-15T19:34:04Z Gsawgwikiadmin 1 Created page with "Template for spectral follow-up of Gaia targets. Title: Spectroscopic classification of Gaia, ASAS-SN and TOCP transients with the WHT ISIS. Authors: H. Campbell (Univers..." wikitext text/x-wiki Template for spectral follow-up of Gaia targets. Title: Spectroscopic classification of Gaia, ASAS-SN and TOCP transients with the WHT ISIS. Authors: H. Campbell (University of Cambridge), T. Wevers (RU Nijmegen), M. Fraser (University of Cambridge), P. G. Jonker (SRON & RU Nijmegen), L. Wyrzykowski (Warsaw Observatory), S. Hodgkin, N. Blagorodnova (University of Cambridge) Text: We report spectroscopic confirmation and classifications for reported Gaia Photometric Science Alerts (http://gaia.ac.uk/selected-gaia-science-alerts), together with targets from the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al. 2014) and the TOCP list. All spectra were taken with the 4.2m William Herschel Telescope on La Palma, over the nights of 11 to 12 June. Low resolution spectra were taken using ISIS with the R158R and R300B gratings. The classifications were done with SNID (Blondin and Tonry 2007, ApJ, 666, 1024). Name RA Dec Date Classification Comments Gaia15agj 03:11:11.50 +37:58:2.10 2015-06-11 SN Ia At max, z=0.04 (also classified in ATEL 7623) Gaia15ada 11:41:02.05 +65:02:33.3 2015-06-11 SN IIP Normal IIP mid-plateau, z=0.04 (aka ps15ye) Gaia15agh 12:04:05.11 +14:04:04.9 2015-06-11 SN Ia +2 weeks, z=0.04 Gaia15adt 14:01:14.96 +44:18:29.8 2015-06-11 SN Ia +2 months, z=0.06 Gaia15adn 14:17:00.71 +62:54:42.9 2015-06-11 SN Ia +2 months, z=0.04 Gaia15adh 17:12:30.88 +48:28:11.9 2015-06-11 SN Ia +3 months, z=0.06 Gaia15aew 22:43:02.60 +49:54:49.0 2015-06-11 Stellar Balmer absorption Gaia15aeq 23:31:29.42 +24:16:34.7 2015-06-11 SN Ia +1.5 months, z=0.07 Gaia15aez 23:31:27.58 +22:50:58.4 2015-06-11 SN II z=0.07 (Broad H alpha emission seen in low S/N spectrum) Gaia15aeu 11:00:37.85 -11:56:47.6 2015-06-12 Stellar Red with strong narrow Na D absorption. ASASSN_15ku 10:44:22.06 +18:34:59.5 2015-06-12 CV Broad wing Halpha absorption, with filled in core from narrow emission Gaia15Aagc 12:18:23.70 +35:35:24.0 2015-06-12 SN Ia +2 weeks, z=0.04 Gaia15adl 16:41:16.95 +39:17:28.7 015-06-12 CCSN Broad nebular emission lines, including [Ca] and [O] at z=0.03 (consistent with MCG +7-34-134) Gaia15afr 23:29:33.60 +39:34:22.7 2015-06-12 SN II Broad Halpha emission, z=00.03 Gaia15agf 22:02:29.36 -20:19:46.0 2015-06-12 SN Ia +2 weeks, z=0.06 ASASSN_15kw 17:19:37.10 +04:31:23.8 2015-06-12 CV Strong Halpha in emission, FWHM ~1200km\s from Lorentzian fit. Also HeII emission at 5876 PSN J14372160+3634018 14:37:21.60 +36:34:01.8 2015-06-12 SN II Shows broad Halpha, consistent with a Type II SN soon after explosion. We acknowledge ESA Gaia (cosmos.esa.int/gaia), and the DPAC Photometric Science Alerts Team (http://gaia.ac.uk/selected-gaia-science-alerts). 4e368862e9bca6d3232a9bcba683f8a3ae427786 1989 1985 2015-06-16T10:13:58Z Nadia 27 wikitext text/x-wiki Template for spectral follow-up of Gaia targets. Title: Spectroscopic classification of Gaia, ASAS-SN and TOCP transients with the WHT ISIS. Authors: H. Campbell (University of Cambridge), T. Wevers (RU Nijmegen), M. Fraser (University of Cambridge), P. G. Jonker (SRON & RU Nijmegen), L. Wyrzykowski (Warsaw Observatory), S. Hodgkin, N. Blagorodnova (University of Cambridge) Text: We report spectroscopic confirmation and classifications for reported Gaia Photometric Science Alerts (http://gaia.ac.uk/selected-gaia-science-alerts), together with targets from the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al. 2014) and the TOCP list. All spectra were taken with the 4.2m William Herschel Telescope on La Palma, over the nights of 11 to 12 June. Low resolution spectra were taken using ISIS with the R158R and R300B gratings. The classifications were done with SNID (Blondin and Tonry 2007, ApJ, 666, 1024). <pre> Name | RA (J2000) | Dec (J2000) | Disc. Source | Disc. Date | Disc Mag | z | Type | Phase | Notes<br> Gaia15agj | 03:11:11.50 | +37:58:2.10 | Gaia | 2015-06-03 | 18.49 G | 0.04 | SN Ia | Max | Also classified in ATEL #7623 PSN J14372160+3634018 | 14:37:21.60 |+36:34:01.8 | CBET | 2015-06-12 | | 0.014093 | SN II | +5d | (1) </pre> <p> (1) Shows broad Halpha, consistent with a Type II SN soon after explosion. </p> We acknowledge ESA Gaia (cosmos.esa.int/gaia), and the DPAC Photometric Science Alerts Team (http://gaia.ac.uk/selected-gaia-science-alerts). ae5c4a3333e643ffa81a0a32533e969263401d6a 1990 1989 2015-06-16T10:19:40Z Nadia 27 wikitext text/x-wiki Template for spectral follow-up of Gaia targets. Title: Spectroscopic classification of Gaia, ASAS-SN and TOCP transients with the WHT ISIS. Authors: H. Campbell (University of Cambridge), T. Wevers (RU Nijmegen), M. Fraser (University of Cambridge), P. G. Jonker (SRON & RU Nijmegen), L. Wyrzykowski (Warsaw Observatory), S. Hodgkin, N. Blagorodnova (University of Cambridge) Text: We report spectroscopic confirmation and classifications for reported Gaia Photometric Science Alerts (http://gaia.ac.uk/selected-gaia-science-alerts), together with targets from the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al. 2014) and the TOCP list. All spectra were taken with the 4.2m William Herschel Telescope on La Palma, over the nights of 11 to 12 June. Low resolution spectra were taken using ISIS with the R158R and R300B gratings. The classifications were done with SNID (Blondin and Tonry 2007, ApJ, 666, 1024). <pre> Name | RA (J2000) | Dec (J2000) | Disc. Source | Disc. Date | Disc Mag | z | Type | Phase | Notes<br> Gaia15agj | 03:11:11.50 | +37:58:2.10 | Gaia | 2015-06-03 | 18.49 G | 0.04 | SN Ia | Max | Also classified in ATEL #7623 PSN J14372160+3634018 | 14:37:21.60 |+36:34:01.8 | CBET | 2015-06-12 | | 0.014093 | SN II | +5d | (1) </pre> <p> (1) Shows broad Halpha, consistent with a Type II SN soon after explosion. </p> We acknowledge ESA Gaia (cosmos.esa.int/gaia), and the DPAC Photometric Science Alerts Team (http://gaia.ac.uk/selected-gaia-science-alerts). cfd1ad305f2a1fcf7824c42acf098e4b9df2bfac 1991 1990 2015-06-16T11:01:04Z Nadia 27 wikitext text/x-wiki Template for spectral follow-up of Gaia targets. Title: Spectroscopic classification of Gaia, ASAS-SN and TOCP transients with the WHT ISIS. Authors: H. Campbell (University of Cambridge), T. Wevers (RU Nijmegen), M. Fraser (University of Cambridge), P. G. Jonker (SRON & RU Nijmegen), L. Wyrzykowski (Warsaw Observatory), S. Hodgkin, N. Blagorodnova (University of Cambridge) Text: We report spectroscopic confirmation and classifications for reported Gaia Photometric Science Alerts (http://gaia.ac.uk/selected-gaia-science-alerts), together with targets from the All-Sky Automated Survey for Supernovae (ASAS-SN; Shappee et al. 2014) and the TOCP list. All spectra were taken with the 4.2m William Herschel Telescope on La Palma, over the nights of 11 to 12 June. Low resolution spectra were taken using ISIS with the R158R and R300B gratings. The classifications were done with SNID (Blondin and Tonry 2007, ApJ, 666, 1024). <pre> <pre> Name | RA (J2000) | Dec (J2000) | Disc. Source | Disc. Date | Disc Mag | z | Type | Phase | Notes<br> Gaia15agj | 03:11:11.50 | +37:58:2.10 | Gaia | 2015-06-03 | 18.49 G | 0.04 | SN Ia | Max | (2) PSN J14372160+3634018 | 14:37:21.60 | +36:34:01.8 | CBET | 2015-06-12 | 17.7 | 0.014093 | SN II | Max | (1) </pre> </pre> <pre> <p> (1) Also classified in ATEL #7623 (2) Shows broad Halpha, consistent with a Type II SN soon after explosion. </p> </pre> We acknowledge ESA Gaia (cosmos.esa.int/gaia), and the DPAC Photometric Science Alerts Team (http://gaia.ac.uk/selected-gaia-science-alerts). c79d7acf61dfa8d6dbe8d0d9eaf14c9ba2afd933 0 253 1986 2015-06-15T19:41:12Z Gsawgwikiadmin 1 Created page with "Template ATEL reporting photometric follow-up of Gaia alerts without Gaia people. Title: Gaia15agj in edge-on galaxy SDSS J095058.70+375758.8 confirmed by Mercator/Maia im..." wikitext text/x-wiki Template ATEL reporting photometric follow-up of Gaia alerts without Gaia people. Title: Gaia15agj in edge-on galaxy SDSS J095058.70+375758.8 confirmed by Mercator/Maia imaging Author: R. I. Anderson (Physics and Astronomy Department, The Johns Hopkins University, Baltimore, MD, USA), L. Palaversa, N. Mowlavi, L. Eyer (Department of Astronomy, University of Geneva, Switzerland) We report confirmation of <a href="http://gaia.ac.uk/selected-gaia-science-alerts" name="Gaia Science Alerts" title="Gaia Science Alerts">Gaia Science Alerts</a> transient Gaia15agj, detected by Gaia satelite on 2015 Jun 03 ca. 05 UT. Images were obtained in U, G, and R bands of the Maia instrument mounted to the Flemish 1.2m Mercator telescope at Roque de los Muchachos observatory, La Palma, Canary Islands, Spain, on 2015 June 09 ca. 21UT. <a href="http://obswww.unige.ch/wordpress/variabilite/files/2015/02/Gaia15agj.png" name="Gaia15agj">Gaia15agj</a> is located approximately 6.8 arcsec to the East (= 5.5 kpc for 0.806 kpc/arcsec from NED) of the center of edge-on galaxy SDSS J095058.70+375758.8 = FGC 0955 = GALEXASC J095059.00+375759.7 which has a redshift of z=0.04 (from NED). SIMBAD identifies this galaxy as Active Galactic Nucleus 2MFGC 7622. Gaia15agj was measured at the apparent magnitudes listed in the table below. These translate to absolute magnitudes of approximately (-18.4, -19.21, -19.61) in U, G, and R bands, respectively, assuming A_&lambda; of 0.076, 0.059, and 0.041 in the SDSS u, g, and r filters and distance modulus (m-M) = 36.11 +/- 0.15 mag (both from NED). This new source is not present in archival 2MASS/DSS/SDSS images. The location of the transient off-center in an Sc galaxy renders it a likely supernova candidate. MAIA G band 400x400 pixel cut-out image is provided (N is up, E is left and scale is 0.276"/pix). <nowiki> <table style="width:40%" border="1px solid black" padding="10"> <tr align="center"> </td> <td colspan=2> MJD</td> <td colspan=3> Gaia15agj</td> </tr> <tr align="center"> <td>Gaia detection</td> <td>Observed</td> <td>U</td> <td>G</td> <td>R</td> </tr> <tr align="center"> <td>57,176.2</td> <td>57,182.9</td> <td>~17.7</td> <td>~16.9</td> <td>~16.5</td> </tr> </tr> </table> </nowiki> The photometric calibrations were obtained using the <a href="http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Follow-up" name="CPCS">Cambridge Photometric Calibration Server (CPCS)</a>, designed and maintained by Sergey Koposov and Lukasz Wyrzykowski. 9cee78a323889870db992b2c63b412dd6a128692 8 3 1987 1656 2015-06-15T19:44:49Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:rationale|Rationale **workshop2015:agenda|Program **workshop2015:registration|Participants and Registration **workshop2015:logistics|Logistics *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX ad5ef3bd58a515c099929e8619ad3db9047760d7 0 254 1988 2015-06-15T19:45:45Z Gsawgwikiadmin 1 Created page with "Place: Liverpool, UK Dates: 10-13 November 2015" wikitext text/x-wiki Place: Liverpool, UK Dates: 10-13 November 2015 21fc9c393c8931eda119f91e377bf52c6f985df2 0 255 1992 2015-06-18T09:51:57Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2015.jpg|right|300px|Poster]] '''The sixth Gaia Science Alerts workshop will be held in Workshop2015:logistics | Liverpool on 10-13 November 201..." wikitext text/x-wiki == Welcome! == [[File:Poster2015.jpg|right|300px|Poster]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * TBD LOC: * TBD 25655576b3100423ef3ec5d8166d7170620cc14a 1995 1992 2015-06-19T13:48:21Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2015.jpg|right|300px|Poster]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak 0838b01eb20c0b3fcaa76b05b5bc581d8f3f3d33 1997 1995 2015-06-24T09:09:30Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2015.jpg|right|300px|Poster]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] REGISTRATION NOW OPEN! * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak b012f5e5f9bd41e159d605038852653d9b261893 0 1 1993 1655 2015-06-18T21:26:04Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Structure == <center> '''We are now creating the substructure WGs concentrating on broad science goals. See [[Working groups]] for details.''' </center> ---- == Workshops == <center> '''<Big>[[Workshop2015:main|6th Gaia Science Alerts Workshop 2015, Liverpool]]</Big>''' </center> ---- <center> [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2015, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- ee05cb18c304cc02a3d128b873d95adc39828213 0 256 1994 2015-06-19T11:29:26Z Gsawgwikiadmin 1 Created page with "Registration is now open! [http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]" wikitext text/x-wiki Registration is now open! [http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE] 86dc05c8292a46cb4640c3944049e5b3feb6ab10 1996 1994 2015-06-19T19:37:11Z Gsawgwikiadmin 1 wikitext text/x-wiki '''Registration is now open! Registration will close 30 September 2015. ''' [http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE] Contact: gaiasciencealertsworkshop2015@gmail.com 5f5af9826ab1593be86ab05e9ffb54f9bec22c9d 2001 1996 2015-06-30T19:24:23Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' [http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE] Contact: gaiasciencealertsworkshop2015@gmail.com 1cbeed568a9e6f14b1259a13a21bbf64318f67b3 0 257 1999 2015-06-30T19:18:19Z Gsawgwikiadmin 1 Created page with "Gaia was launched in December 2013 and began science operations in August 2014. While the first superb astrometric data will be delivered to the community in coming years, Gai..." wikitext text/x-wiki Gaia was launched in December 2013 and began science operations in August 2014. While the first superb astrometric data will be delivered to the community in coming years, Gaia Photometric Science Alerts has been publishing alerts since October 2014. So far, about 300 transients have been found, among them many supernovae, cataclysmic variables, candidate microlensing events as well as rare and exciting discoveries (e.g., the eclipsing AM CVn Gaia14aae). Many Gaia alerts have been followed-up spectroscopically and photometrically, with the Gaia Follow-up Network alone collecting nearly 10,000 photometric data points for Gaia triggers. We would like to gather together again this year in [[Workshop2015:logistics | Liverpool (UK) on 10-13 November 2015]] to talk about the first year of the Gaia Science Alerts programme. Topics for the meeting include: * Discussion of the extensive follow-up observations carried out over the past year. * Using these data to aid automated classification within the AlertPipe software. * The new Gaia Alerts publisher and interfaces. * Science cases for Gaia Science Alerts. * The next steps: how to exploit improved performance, and organise the follow-up. * Interfaces to robotic telescope networks. * Feedback from follow-up into Gaia Alerts. * Outreach Opportunities. * Interfacing to other Alert streams. * Dedicated hands-on sessions: ** Introduction of Gaia Alerts to new follow-up partners. ** Tools for processing and analysing follow-up photometry and spectroscopy. ---- As with previous meetings, we are happy to announce the support of the EC OPTICON network for this year’s workshop (under WP11: Time-domain Astronomy) 1e9f69df7d59fda66cda5feaf23a4df894f5ec03 0 258 2000 2015-06-30T19:23:34Z Gsawgwikiadmin 1 Created page with "We plan to start the meeting with lunch on Tuesday the 10th of November and finish with lunch on Friday 13th Nov. Detailed agenda will be composed of suggested contributions...." wikitext text/x-wiki We plan to start the meeting with lunch on Tuesday the 10th of November and finish with lunch on Friday 13th Nov. Detailed agenda will be composed of suggested contributions. Friday morning will probably be dedicated to the hands-on session and/or splinters. 4d012b7f6bfce0595bb905ab39b61dfae356cdec 0 256 2002 2001 2015-07-16T22:20:29Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' [http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE] Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu '''If you have registered, but don't see your name here within a week, do email us!''' 78d337622d447a98af3174824f13b2cb36030cb1 2003 2002 2015-07-16T22:20:47Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' [http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE] Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu '''If you registered, but don't see your name here within a week, do email us!''' ccb6ccf4579d2fc7c9b094de25ebfe0208f87822 2004 2003 2015-07-16T22:21:07Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu '''If you registered, but don't see your name here within a week, do email us!''' 38b3a8afa854e46f4d4d98c21af78e81fd773304 2005 2004 2015-07-16T22:21:21Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu '''If you registered, but don't see your name here within a week, do email us!''' deeafff5a528ac843497e122cf93a62289c56335 2006 2005 2015-07-22T12:46:44Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb '''If you registered, but don't see your name here within a week, do email us!''' ac38199f6c4d1ac75c28432faed09236617321d9 2007 2006 2015-07-23T17:17:51Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema '''If you registered, but don't see your name here within a week, do email us!''' bd02be081be846eb022aa566f0fe3bf891c48b5c 2008 2007 2015-07-29T11:29:53Z Zuzanna 36 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco '''If you registered, but don't see your name here within a week, do email us!''' 49c44d95d14339d644e9c41280edd72ccafdda9e 0 1 2009 1993 2015-07-29T11:30:21Z Zuzanna 36 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Structure == <center> '''We are now creating the substructure WGs concentrating on broad science goals. See [[Working groups]] for details.''' </center> ---- == Workshops == <center> '''<Big>[[Workshop2015:main|6th Gaia Science Alerts Workshop 2015, Liverpool]]</Big>''' </center> ---- <center> [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 23d572b547b83cf0007df3083a5a76c26ca73ced 0 254 2010 1988 2015-07-29T20:36:16Z Gsawgwikiadmin 1 wikitext text/x-wiki Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 a2562bc070313912f6ed192004562db5c5b0ea64 2012 2010 2015-08-05T10:35:38Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. <br>There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station. A combined bus/train ticket to Liverpool can be purchased at the airport. The bus services direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=outbound ( 500 )], [http://www.merseyrail.org/media/95000/86A%20Liverpool%20-%20Liverpool%20John%20Lennon%20Airport%20%28from%2016%20September%202012%29.pdf ( 86, 86A, 86D, 86E] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=outbound ( 80, 80A ) ]. <br> These are operated by Arriva Bus and also go via Liverpool South Parkway station. Journey time to Liverpool is about 30 minutes. === MAN - Manchester Airport === [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. <br>There is a rail link at this station with trains operated by Northern Rail direct to Liverpool Lime Street station leaving every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf (Timetable)]. The journey time to Liverpool is approximately 1 hour. 1bd5f6c8aea757c82c277e131d26d0a0cc691984 2013 2012 2015-08-05T10:37:11Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. <br>There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station. A combined bus/train ticket to Liverpool can be purchased at the airport. The bus services direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=outbound 500 ], [http://www.merseyrail.org/media/95000/86A%20Liverpool%20-%20Liverpool%20John%20Lennon%20Airport%20%28from%2016%20September%202012%29.pdf 86, 86A, 86D, 86E] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=outbound 80, 80A ]. <br> These are operated by Arriva Bus and also go via Liverpool South Parkway station. Journey time to Liverpool is about 30 minutes. === MAN - Manchester Airport === [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. <br>There is a rail link at this station with trains operated by Northern Rail direct to Liverpool Lime Street station leaving every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf (Timetable)]. The journey time to Liverpool is approximately 1 hour. 17e4f88be5728858f44e24acedee4ad1603b6b95 2014 2013 2015-08-05T11:04:00Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. <br>There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT near the city. <br>Liverpool South Parkway is a double railway station providing two separate routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by Arriva and also go via Liverpool South Parkway station. Journey time to Liverpool is about 30 minutes. === MAN - Manchester Airport === [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. <br>There is a rail link at this station. Trains operated by Northern Rail go direct to Liverpool Lime Street station leaving every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf (Timetable)]. The journey time to Liverpool is approximately 1 hour. d846f7c9474bbd19638edf3c6043c8cce18a3602 2015 2014 2015-08-05T11:26:03Z A.Piascik 40 Basic Air/Train/Bus travel details added wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. <br>There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT near the city. <br>Liverpool South Parkway is a double railway station providing two separate routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is about 30 minutes. === MAN - Manchester Airport === [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. <br>There is a rail link at this station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf (Timetable)]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly station and changing there for a train to Liverpool Lime Street. <br>This journey time is approximately 1.5 hours The [http://www.nationalrail.co.uk/ Rail Journey Planner] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. 789db3de04eafd10e16093fb624e4e1925d11cab 2016 2015 2015-08-05T11:55:34Z A.Piascik 40 /* MAN - Manchester Airport */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. <br>There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT near the city. <br>Liverpool South Parkway is a double railway station providing two separate routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is about 30 minutes. === MAN - Manchester Airport === [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. <br>There is a rail link at this airport. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf (Timetable)]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly station and changing there for a train to Liverpool Lime Street. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. The [http://www.nationalrail.co.uk/ Rail Journey Planner] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. 750d2c1fef6abddc3d9927f2089f5bba85fbbbc9 2017 2016 2015-08-05T12:08:52Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. <br>There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT near the city. <br>Liverpool South Parkway is a double railway station providing two separate routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. === MAN - Manchester Airport === [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. <br>There is a rail link at this airport. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf (Timetable)]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly station and changing there for a train to Liverpool Lime Street. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. c4640004034a19cd62a240cd518bb67a3179748f 2018 2017 2015-08-05T13:39:43Z A.Piascik 40 /* Airports */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. === MAN - Manchester Airport === * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. There is a rail link at this airport. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly station and changing there for a train to Liverpool Lime Street. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. == Railway == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. Eurostar trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains]. The journey from Euston to Liverpool takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. 4986a469139987974f4f57a7f0a81c2a4060c257 2019 2018 2015-08-05T13:54:03Z A.Piascik 40 Updated train section wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. === MAN - Manchester Airport === * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf, see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Railway == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. Eurostar trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains]. The journey from Euston to Liverpool takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. bc4bab0730d8bb65a933f9f402ef8717265afb1a 2020 2019 2015-08-05T13:59:27Z A.Piascik 40 /* Railway */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel Info = == Airports == There are two airports providing access to the city of Liverpool. === LPL - Liverpool John Lennon Airport === * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. === MAN - Manchester Airport === * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf, see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Railway == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. Eurostar trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. 0f3a0dd419df782a46ea3e5225686016a016d86f 2021 2020 2015-08-05T14:17:20Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 = Travel = == Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. a3bb9020abde267bb1ef40715ab382d5a61b8fd0 2023 2021 2015-08-05T15:02:54Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in blue. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. = Travel = == Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and also go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. 753582160d9305eae9a3ca7cb5d84ba8a9de55f8 2024 2023 2015-08-05T15:18:40Z A.Piascik 40 Minor mod - Arrivabus 500 does not go via South Parkway wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in blue. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. = Travel = == Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. 373166794cf884b51cb8681871563b54f8ded562 2026 2024 2015-08-05T16:51:36Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in blue. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. = Travel = == Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == Car Parking == [[File:Gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked in blue and red, is very expensive per day. The multi-story marked <b><font color="red">P</font></b> is recommended at £4.00 per day and it is a 5 minute walk to the Gaia venue. It is Pay-and-Display and open 7:00am until 20:00pm, motorcycles and disabled are free. The open air car-park opposite marked <b><font color="green">P</font></b> will normally have free spaces if the multi-storey is full. More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 8c0bb8ff005e351db9c4b4ad17d341a482958690 2028 2026 2015-08-06T07:01:06Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in blue. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. = Travel = == Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked in blue and red, is very expensive per day. The multi-story marked <b><font color="red">P</font></b> is recommended at £4.00 per day and it is a 5 minute walk to the Gaia venue. It is Pay-and-Display and open 7:00am until 20:00pm, motorcycles and disabled are free. The open air car-park opposite marked <b><font color="green">P</font></b> will normally have free spaces if the multi-storey is full. More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 2cf65cd22f6f07c1765a71ca64ea11da8b118a01 2034 2028 2015-08-06T07:42:12Z A.Piascik 40 Added icons. Updated parking. Minor corrections. wikitext text/x-wiki = Location Info = Place: Liverpool, UK Venue: Open Labs next to the Astrophysics Research Institute Dates: 10-13 November 2015 [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. d280f29d7b8dbdec021c127c5ecf7938a69cd7e9 2035 2034 2015-08-06T09:25:03Z Rob.barnsley 42 /* Location Info */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ eaysJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. eed919a342c7057024695361c2fb7d96cb650a6d 2036 2035 2015-08-06T15:40:41Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ easyJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. <br>A combined bus/train ticket can be purchased at the airport. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. cf4c59198ed6851991e42aa465a9d7801628fd01 2037 2036 2015-08-06T16:21:45Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The principle airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ easyJet, Ryanair, Blue Air, Flybe Wizz Air, Czech, Thomson and Aer Lingus]. There is no rail link at this airport but there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes to Liverpool Lime Street or Liverpool Central stations, which are in the city. If arriving after 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. SaveAway ticket for [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] costs £3.90. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br> These are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva]. The 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ principle airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are some trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston, where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute by walking or via the London Underground on the Victoria Line (pale blue) or Northern Line (black). <br>Direct trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 61261c31119adeb1e63d0720861e4f6208ecd9af 2038 2037 2015-08-06T18:20:20Z A.Piascik 40 Recreating edits after they mysteriously disappeared. wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ easyJet, Ryanair, Blue Air, Flybe, Wizz Air, Czech, Thomson and Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. A SaveAway ticket for including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for travel to destinations in the city of Liverpool and costs £3.90. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br>Buses are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and the 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <b><font color="#0583d2">Victoria Line</b> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 2018ef53c76167c1423d985e17fd0fb40bf3d331 2039 2038 2015-08-07T10:18:42Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The airlines flying to this airport are [http://www.liverpoolairport.com/flight-information/airlines/ easyJet, Ryanair, Blue Air, Flybe, Wizz Air, Czech, Thomson and Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. A SaveAway ticket for including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for travel to destinations in the city of Liverpool and costs £3.90. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br>Buses are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and the 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. ca663af46b83b396416a09713bbabf7378549b75 2040 2039 2015-08-07T10:30:55Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The [http://www.liverpoolairport.com/flight-information/airlines/ airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson], [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. A SaveAway ticket for including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for travel to destinations in the city of Liverpool and costs £3.90. The bus services from the airport direct to Liverpool are numbered [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A ]. <br>Buses are operated by [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] and the 80A & 86A services go via Liverpool South Parkway station. Journey time to Liverpool is approximately 30 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. d2f705111787c55827045831a8f951b6c2f1f14b 2041 2040 2015-08-07T10:46:59Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The [http://www.liverpoolairport.com/flight-information/airlines/ airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson], [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for travel to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A]. <br>Services 80A & 86A go via Liverpool South Parkway station. The journey time into Liverpool is approximately 25-45 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 24651013e338f22f782cf7b778fa69750f3cfda4 2042 2041 2015-08-07T10:48:09Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. The [http://www.liverpoolairport.com/flight-information/airlines/ airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson], [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] suitable for travel to destinations in the city of Liverpool costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] and [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A]. <br>Services 80A & 86A go via Liverpool South Parkway station. The journey time into Liverpool is approximately 25-45 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 23efee9279900e9f22450a86a841bf9ee91fb427 2043 2042 2015-08-07T10:53:59Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airports == There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] suitable for travel to destinations in the city of Liverpool costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway station. Click on numbers to view routes and stopping points. The journey time into Liverpool is approximately 25-45 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. a8145506563366592fef0c89f54e486136d5957b 2044 2043 2015-08-07T11:16:30Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] suitable for travel to destinations in the city of Liverpool costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway station. <br>Click on numbers to view routes and stopping points. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. The journey time into Liverpool is approximately 25-45 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 76128b4de8d0b2a20724f6fdd963bc2a53e8f9bc 2045 2044 2015-08-07T11:19:19Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] suitable for travel to destinations in the city of Liverpool costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500 ], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway station. Click on numbers to view routes and stops. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains] and the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability. Tickets can be collected at the departure station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail] and the stations in and around the city can be view via the link to [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. e970fc9b0f40760846c9be9089ed4485dd3a4837 2046 2045 2015-08-07T11:34:44Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is NOT in the city. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] suitable for travel to destinations in the city of Liverpool costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway station. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. A taxi from Manchester airport to Liverpool city centre costs around £60 == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. e0945770dd7422d533e20797a722296ab2764808 2047 2046 2015-08-07T11:36:35Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] suitable for travel to destinations in the city of Liverpool costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway station. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. A taxi from Manchester airport to Liverpool city centre costs around £60 == [[File:icon_train.png | 32px | middle ]] Rail Travel == * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station located in the city. There are a few trains direct from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS] but most require a change at Crewe [CRE] station. <br>The quickest trains from London Euston to Liverpool Lime Street are operated by [http://www.virgintrains.co.uk/ Virgin Trains], the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest tickets are [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ Advance] booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a 5 minute walk or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. b4fa570b08cc5352e1f6af74e7c28b39aa1753f6 2048 2047 2015-08-07T13:43:39Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus/train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for travel to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway station. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour, [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf see Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and changing there for a train to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. It accepts three letter abbreviation [TLA] station names. A taxi from Manchester airport to Liverpool city centre costs around £60 == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. [http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require a change at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. ca617cd31cf746f03e47c3d51ba791f76b25355a 2049 2048 2015-08-10T09:06:47Z A.Piascik 40 /* 32px | middle Airport Travel */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times, you can enter three letter abbreviation [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. [http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require a change at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a 5 minute walk from the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 4e7731fdfa5dcb99000f3dbc17a0fbef7a9c8a78 2050 2049 2015-08-10T09:20:14Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times, you can enter three letter abbreviation [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. [http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and it is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. a32e78a51f3eb73798a6aa101bb07fbd17311c80 2051 2050 2015-08-10T09:22:52Z A.Piascik 40 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times, you can enter three letter abbreviation [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and it is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 59d4a892d49d59e66cf7c587998b0974fd84c1b5 0 255 2011 1997 2015-07-29T20:56:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2015.jpg|right|300px|Poster]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] REGISTRATION NOW OPEN! * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat d6ed342f0bd9a82b24cf9acb54f3984b2a08887f 6 259 2022 2015-08-05T14:52:05Z A.Piascik 40 gaia 2015 venue, ARI and city stations wikitext text/x-wiki gaia 2015 venue, ARI and city stations 2dcf4776e9f5e5c9786d31fa2994098cf71b2b85 6 260 2025 2015-08-05T16:21:40Z A.Piascik 40 Recommended car parking wikitext text/x-wiki Recommended car parking 959a1b946bbaa46ab35e2bc76949682b15c10c0b 2027 2025 2015-08-06T06:59:40Z A.Piascik 40 A.Piascik uploaded a new version of [[File:Gaia2015parking.png]] wikitext text/x-wiki Recommended car parking 959a1b946bbaa46ab35e2bc76949682b15c10c0b 6 261 2029 2015-08-06T07:03:13Z A.Piascik 40 airplane icon wikitext text/x-wiki airplane icon 90b8b613acb4282854677f40f0c4bb954dd55dd9 6 262 2030 2015-08-06T07:14:58Z A.Piascik 40 bus icon wikitext text/x-wiki bus icon 462ef3f2c82d6244d53ec57b51967201286f1e64 6 263 2031 2015-08-06T07:15:32Z A.Piascik 40 icon train wikitext text/x-wiki icon train 82c70d624a132e5325dc14abc0785bffcfda7fbd 2032 2031 2015-08-06T07:15:51Z A.Piascik 40 A.Piascik uploaded a new version of [[File:Icon car.png]] wikitext text/x-wiki icon train 82c70d624a132e5325dc14abc0785bffcfda7fbd 6 264 2033 2015-08-06T07:17:07Z A.Piascik 40 icon train wikitext text/x-wiki icon train 82c70d624a132e5325dc14abc0785bffcfda7fbd 0 254 2052 2051 2015-08-10T09:25:21Z A.Piascik 40 /* MAN - Manchester Airport */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although here is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and it is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. d971a60034e52b60b097dba330f4a935955a53de 2053 2052 2015-08-13T09:00:12Z A.Piascik 40 /* LPL - Liverpool John Lennon Airport */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs next to the Astrophysics Research Institute [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The location of the Astrophysics Research Institute is marked in blue and the provisional Gaia 2015 venue is marked in red. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and it is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. 9a598d9c954cc4cbc6f8a1bc4196f49f9d05b70b 2054 2053 2015-08-13T12:30:46Z A.Piascik 40 /* Location Info */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs located in the IC1 building close to the [http://www.astro.ljmu.ac.uk/Main_Page Astrophysics Research Institute] &nbsp;&nbsp;[https://www.ljmu.ac.uk/contact-us/find-us/directions-jlad-and-im/open-labs-ic1-science-park IC1 Liverpool Science Park]<br> &nbsp;&nbsp;131 Mount Pleasant<br> &nbsp;&nbsp;Liverpool<br> &nbsp;&nbsp;L3 5TF<br> &nbsp;&nbsp;United Kingdom<br> &nbsp;&nbsp;+44 (0)151 705 3400<br> [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Gaia Workshop 2015 venue is marked in <font color="#db4436">red</font>. The Astrophysics Research Institute is on the 2^nd floor of the building marked in <font color="#3f5ba9">blue</font>. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and it is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. e515022a9a18c4723cd3bb5395ef6edc0cab071f 2062 2054 2015-08-20T13:51:23Z H.Jermak 41 wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs located in the IC1 building close to the [http://www.astro.ljmu.ac.uk/Main_Page Astrophysics Research Institute] &nbsp;&nbsp;[https://www.ljmu.ac.uk/contact-us/find-us/directions-jlad-and-im/open-labs-ic1-science-park IC1 Liverpool Science Park]<br> &nbsp;&nbsp;131 Mount Pleasant<br> &nbsp;&nbsp;Liverpool<br> &nbsp;&nbsp;L3 5TF<br> &nbsp;&nbsp;United Kingdom<br> &nbsp;&nbsp;+44 (0)151 705 3400<br> [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Gaia Workshop 2015 venue is marked in <font color="#db4436">red</font>. The Astrophysics Research Institute is on the 2^nd floor of the building marked in <font color="#3f5ba9">blue</font>. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and it is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. <br clear="all"> =Accommodation= A large variety of hotels, hostels and B&Bs are available in Liverpool centre. Below are a selection of hotels that offer a discounted rate for the conference. There are generally 20 rooms reserved per large hotel (unless otherwise stated), most require telephone payments or payment on arrival. [http://www.daysinn.co.uk/hotels/united-kingdom/liverpool/days-inn-liverpool-city-centre/hotel-overview Days Inn Liverpool] The Days Inn hotel is located near the River Mersey and the Docks area (~5-10 minute walk) and from the city centre (<5 min walk). It is also next to James Street Station which can be directly accessed on the [http://www.merseyrail.org/ Mersey Rail Network] underground trains from Lime Street (a return or single from Lime Street to James Street costs less than £2). It is a ~20 minute walk from this hotel to the conference building. Parking is available nearby but isn’t cheap [http://www.q-park.co.uk/parking/parkingid/582 Q park]. To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are 20 rooms reserved at this rate from 9-13 November 2015 and will be available to book exclusively for the conference if booked before the end of September. After that the prices may be subject to change or rooms unavailable. Guests are able to book by calling 0151 203 1910 (option 1) Monday to Friday between 9am and 5pm or can email here reservations@daysinnliverpool.com. <br>&nbsp;&nbsp;£50 per night single occupancy (with Breakfast) <br>&nbsp;&nbsp;£60 per night double/twin occupancy (with Breakfast) [http://www.feathers.uk.com/feathers-hotel/ BEST WESTERN Feathers Liverpool Hotel] <br>0151 709 9655 <br>email :feathersreservations@feathers.uk.com The Feathers hotel is very close to the conference venue (~1 minute away). It is ~15 minute walk from Liverpool Lime Street station and from the centre of Liverpool. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are approximately 20 rooms being held for the conference. <br>&nbsp;&nbsp;Double for single occupancy: £69.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Double for double occupancy: £79.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for sole occupancy £84.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for double occupancy £89.95 (inc. breakfast and WiFi) [http://www.aachenhotel.co.uk/ Aachen Hotel], <br>89-91 Mount Pleasant <br>Liverpool <br>L3 5TB <br>T: +44 (0)151 709 3477 <br>T: +44 (0)151 709 3633 The Aachen Hotel is a small hotel on the same street as the conference venue (~5 min walk). There are no rooms reserved due to the size of the hotel but if you quote GAIA LIVERPOOL you can receive the discounted rate. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). <br>&nbsp;&nbsp;£59 for a twin/double room [http://www.accorhotels.com/gb/hotel-7332-aparthotel-adagio-liverpool-city-centre/index.shtml Adagio Aparthotel Liverpool City Centre] <br>1 Fairclough Street <br>L1 1FS Liverpool <br>email : h7332-sl@adagio-city.com The Adagio Aparthotel is next to Liverpool Central Station (accessible via the Wirral line, one stop from Liverpool Lime street station). It is ~15 minute walk from here to the conference venue and the hotel is right in the middle of the city centre. Please contact the hotel directly via the email address above to book at these rates and quote GAIA LIVERPOOL. <br>&nbsp;&nbsp;Studio apartment for sole occupancy - £65 B&B <br>&nbsp;&nbsp;Studio apartment for double occupancy - £75 B&B There are both studio apartments with double and twin beds (limited number of twins). d4497c20c6e51828d6ada6f88e2156b11ce2cebc 2079 2062 2015-10-14T15:12:39Z A.Piascik 40 Added clickable E-mail links. Added a couple of tourist visitor links. wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs located in the IC1 building close to the [http://www.astro.ljmu.ac.uk/Main_Page Astrophysics Research Institute] &nbsp;&nbsp;[https://www.ljmu.ac.uk/contact-us/find-us/directions-jlad-and-im/open-labs-ic1-science-park IC1 Liverpool Science Park]<br> &nbsp;&nbsp;131 Mount Pleasant<br> &nbsp;&nbsp;Liverpool<br> &nbsp;&nbsp;L3 5TF<br> &nbsp;&nbsp;United Kingdom<br> &nbsp;&nbsp;+44 (0)151 705 3400<br> [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Gaia Workshop 2015 venue is marked in <font color="#db4436">red</font>. The Astrophysics Research Institute is on the 2^nd floor of the building marked in <font color="#3f5ba9">blue</font>. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Airport Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. <br clear="all"> =Accommodation= A large variety of hotels, hostels and B&Bs are available in Liverpool centre. Below are a selection of hotels that offer a discounted rate for the conference. There are generally 20 rooms reserved per large hotel (unless otherwise stated), most require telephone payments or payment on arrival. [http://www.daysinn.co.uk/hotels/united-kingdom/liverpool/days-inn-liverpool-city-centre/hotel-overview Days Inn Liverpool] The Days Inn hotel is located near the River Mersey and the Docks area (~5-10 minute walk) and from the city centre (<5 min walk). It is also next to James Street Station which can be directly accessed on the [http://www.merseyrail.org/ Mersey Rail Network] underground trains from Lime Street (a return or single from Lime Street to James Street costs less than £2). It is a ~20 minute walk from this hotel to the conference building. Parking is available nearby but isn’t cheap [http://www.q-park.co.uk/parking/parkingid/582 Q park]. To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are 20 rooms reserved at this rate from 9-13 November 2015 and will be available to book exclusively for the conference if booked before the end of September. After that the prices may be subject to change or rooms unavailable. Guests are able to book by calling 0151 203 1910 (option 1) Monday to Friday between 9am and 5pm or can email here reservations@daysinnliverpool.com. <br>&nbsp;&nbsp;£50 per night single occupancy (with Breakfast) <br>&nbsp;&nbsp;£60 per night double/twin occupancy (with Breakfast) [http://www.feathers.uk.com/feathers-hotel/ BEST WESTERN Feathers Liverpool Hotel] <br>0151 709 9655 <br>E-mail: [mailto:feathersreservations@feathers.uk.com feathersreservations@feathers.uk.com] The Feathers hotel is very close to the conference venue (~1 minute away). It is ~15 minute walk from Liverpool Lime Street station and from the centre of Liverpool. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are approximately 20 rooms being held for the conference. <br>&nbsp;&nbsp;Double for single occupancy: £69.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Double for double occupancy: £79.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for sole occupancy £84.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for double occupancy £89.95 (inc. breakfast and WiFi) [http://www.aachenhotel.co.uk/ Aachen Hotel], <br>89-91 Mount Pleasant <br>Liverpool <br>L3 5TB <br>T: +44 (0)151 709 3477 <br>T: +44 (0)151 709 3633 The Aachen Hotel is a small hotel on the same street as the conference venue (~5 min walk). There are no rooms reserved due to the size of the hotel but if you quote GAIA LIVERPOOL you can receive the discounted rate. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). <br>&nbsp;&nbsp;£59 for a twin/double room [http://www.accorhotels.com/gb/hotel-7332-aparthotel-adagio-liverpool-city-centre/index.shtml Adagio Aparthotel Liverpool City Centre] <br>1 Fairclough Street <br>L1 1FS Liverpool <br>E-mail: [mailto:h7332-sl@adagio-city.com h7332-sl@adagio-city.com ] The Adagio Aparthotel is next to Liverpool Central Station (accessible via the Wirral line, one stop from Liverpool Lime street station). It is ~15 minute walk from here to the conference venue and the hotel is right in the middle of the city centre. Please contact the hotel directly via the email address above to book at these rates and quote GAIA LIVERPOOL. <br>&nbsp;&nbsp;Studio apartment for sole occupancy - £65 B&B <br>&nbsp;&nbsp;Studio apartment for double occupancy - £75 B&B There are both studio apartments with double and twin beds (limited number of twins). =Liverpool Culture and History= For general visitor information visit the [http://www.visitliverpool.com/downtime Visiting Liverpool website]. <br>The city has several [http://www.liverpoolmuseums.org.uk/learning/contact.aspx Museums and Art Galleries] with a fine collection of 19th century art. bf137e9966fb81db1ad2cc59796dce05ba09151c 2080 2079 2015-10-15T07:52:31Z A.Piascik 40 Minor mods. Added planetarium link. wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs located in the IC1 building close to the [http://www.astro.ljmu.ac.uk/Main_Page Astrophysics Research Institute] &nbsp;&nbsp;[https://www.ljmu.ac.uk/contact-us/find-us/directions-jlad-and-im/open-labs-ic1-science-park IC1 Liverpool Science Park]<br> &nbsp;&nbsp;131 Mount Pleasant<br> &nbsp;&nbsp;Liverpool<br> &nbsp;&nbsp;L3 5TF<br> &nbsp;&nbsp;United Kingdom<br> &nbsp;&nbsp;+44 (0)151 705 3400<br> [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Gaia Workshop 2015 venue is marked in <font color="#db4436">red</font>. The Astrophysics Research Institute is on the 2^nd floor of the building marked in <font color="#3f5ba9">blue</font>. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Air Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool's so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. <br clear="all"> =Accommodation= A large variety of hotels, hostels and B&Bs are available in Liverpool centre. Below are a selection of hotels that offer a discounted rate for the conference. There are generally 20 rooms reserved per large hotel (unless otherwise stated), most require telephone payments or payment on arrival. [http://www.daysinn.co.uk/hotels/united-kingdom/liverpool/days-inn-liverpool-city-centre/hotel-overview Days Inn Liverpool] The Days Inn hotel is located near the River Mersey and the Docks area (~5-10 minute walk) and from the city centre (<5 min walk). It is also next to James Street Station which can be directly accessed on the [http://www.merseyrail.org/ Mersey Rail Network] underground trains from Lime Street (a return or single from Lime Street to James Street costs less than £2). It is a ~20 minute walk from this hotel to the conference building. Parking is available nearby but isn’t cheap [http://www.q-park.co.uk/parking/parkingid/582 Q park]. To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are 20 rooms reserved at this rate from 9-13 November 2015 and will be available to book exclusively for the conference if booked before the end of September. After that the prices may be subject to change or rooms unavailable. Guests are able to book by calling 0151 203 1910 (option 1) Monday to Friday between 9am and 5pm or can email here reservations@daysinnliverpool.com. <br>&nbsp;&nbsp;£50 per night single occupancy (with Breakfast) <br>&nbsp;&nbsp;£60 per night double/twin occupancy (with Breakfast) [http://www.feathers.uk.com/feathers-hotel/ BEST WESTERN Feathers Liverpool Hotel] <br>0151 709 9655 <br>E-mail: [mailto:feathersreservations@feathers.uk.com feathersreservations@feathers.uk.com] The Feathers hotel is very close to the conference venue (~1 minute away). It is ~15 minute walk from Liverpool Lime Street station and from the centre of Liverpool. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are approximately 20 rooms being held for the conference. <br>&nbsp;&nbsp;Double for single occupancy: £69.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Double for double occupancy: £79.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for sole occupancy £84.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for double occupancy £89.95 (inc. breakfast and WiFi) [http://www.aachenhotel.co.uk/ Aachen Hotel], <br>89-91 Mount Pleasant <br>Liverpool <br>L3 5TB <br>T: +44 (0)151 709 3477 <br>T: +44 (0)151 709 3633 The Aachen Hotel is a small hotel on the same street as the conference venue (~5 min walk). There are no rooms reserved due to the size of the hotel but if you quote GAIA LIVERPOOL you can receive the discounted rate. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). <br>&nbsp;&nbsp;£59 for a twin/double room [http://www.accorhotels.com/gb/hotel-7332-aparthotel-adagio-liverpool-city-centre/index.shtml Adagio Aparthotel Liverpool City Centre] <br>1 Fairclough Street <br>L1 1FS Liverpool <br>E-mail: [mailto:h7332-sl@adagio-city.com h7332-sl@adagio-city.com ] The Adagio Aparthotel is next to Liverpool Central Station (accessible via the Wirral line, one stop from Liverpool Lime street station). It is ~15 minute walk from here to the conference venue and the hotel is right in the middle of the city centre. Please contact the hotel directly via the email address above to book at these rates and quote GAIA LIVERPOOL. <br>&nbsp;&nbsp;Studio apartment for sole occupancy - £65 B&B <br>&nbsp;&nbsp;Studio apartment for double occupancy - £75 B&B There are both studio apartments with double and twin beds (limited number of twins). =Visitor Information= For general visitor information visit the [http://www.visitliverpool.com/downtime Visiting Liverpool website]. <br>The city has several fine [http://www.liverpoolmuseums.org.uk/learning/contact.aspx Museums and Art Galleries] including a [http://www.liverpoolmuseums.org.uk/wml/visit/floor-plans/planetarium.aspx free planetarium]. 419c019e683dfe25945e0996e60dd99ba57600ba 2083 2080 2015-10-19T12:38:17Z A.Piascik 40 /* Visitor Information */ wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs located in the IC1 building close to the [http://www.astro.ljmu.ac.uk/Main_Page Astrophysics Research Institute] &nbsp;&nbsp;[https://www.ljmu.ac.uk/contact-us/find-us/directions-jlad-and-im/open-labs-ic1-science-park IC1 Liverpool Science Park]<br> &nbsp;&nbsp;131 Mount Pleasant<br> &nbsp;&nbsp;Liverpool<br> &nbsp;&nbsp;L3 5TF<br> &nbsp;&nbsp;United Kingdom<br> &nbsp;&nbsp;+44 (0)151 705 3400<br> [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Gaia Workshop 2015 venue is marked in <font color="#db4436">red</font>. The Astrophysics Research Institute is on the 2^nd floor of the building marked in <font color="#3f5ba9">blue</font>. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Air Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool's so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. <br clear="all"> =Accommodation= A large variety of hotels, hostels and B&Bs are available in Liverpool centre. Below are a selection of hotels that offer a discounted rate for the conference. There are generally 20 rooms reserved per large hotel (unless otherwise stated), most require telephone payments or payment on arrival. [http://www.daysinn.co.uk/hotels/united-kingdom/liverpool/days-inn-liverpool-city-centre/hotel-overview Days Inn Liverpool] The Days Inn hotel is located near the River Mersey and the Docks area (~5-10 minute walk) and from the city centre (<5 min walk). It is also next to James Street Station which can be directly accessed on the [http://www.merseyrail.org/ Mersey Rail Network] underground trains from Lime Street (a return or single from Lime Street to James Street costs less than £2). It is a ~20 minute walk from this hotel to the conference building. Parking is available nearby but isn’t cheap [http://www.q-park.co.uk/parking/parkingid/582 Q park]. To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are 20 rooms reserved at this rate from 9-13 November 2015 and will be available to book exclusively for the conference if booked before the end of September. After that the prices may be subject to change or rooms unavailable. Guests are able to book by calling 0151 203 1910 (option 1) Monday to Friday between 9am and 5pm or can email here reservations@daysinnliverpool.com. <br>&nbsp;&nbsp;£50 per night single occupancy (with Breakfast) <br>&nbsp;&nbsp;£60 per night double/twin occupancy (with Breakfast) [http://www.feathers.uk.com/feathers-hotel/ BEST WESTERN Feathers Liverpool Hotel] <br>0151 709 9655 <br>E-mail: [mailto:feathersreservations@feathers.uk.com feathersreservations@feathers.uk.com] The Feathers hotel is very close to the conference venue (~1 minute away). It is ~15 minute walk from Liverpool Lime Street station and from the centre of Liverpool. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are approximately 20 rooms being held for the conference. <br>&nbsp;&nbsp;Double for single occupancy: £69.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Double for double occupancy: £79.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for sole occupancy £84.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for double occupancy £89.95 (inc. breakfast and WiFi) [http://www.aachenhotel.co.uk/ Aachen Hotel], <br>89-91 Mount Pleasant <br>Liverpool <br>L3 5TB <br>T: +44 (0)151 709 3477 <br>T: +44 (0)151 709 3633 The Aachen Hotel is a small hotel on the same street as the conference venue (~5 min walk). There are no rooms reserved due to the size of the hotel but if you quote GAIA LIVERPOOL you can receive the discounted rate. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). <br>&nbsp;&nbsp;£59 for a twin/double room [http://www.accorhotels.com/gb/hotel-7332-aparthotel-adagio-liverpool-city-centre/index.shtml Adagio Aparthotel Liverpool City Centre] <br>1 Fairclough Street <br>L1 1FS Liverpool <br>E-mail: [mailto:h7332-sl@adagio-city.com h7332-sl@adagio-city.com ] The Adagio Aparthotel is next to Liverpool Central Station (accessible via the Wirral line, one stop from Liverpool Lime street station). It is ~15 minute walk from here to the conference venue and the hotel is right in the middle of the city centre. Please contact the hotel directly via the email address above to book at these rates and quote GAIA LIVERPOOL. <br>&nbsp;&nbsp;Studio apartment for sole occupancy - £65 B&B <br>&nbsp;&nbsp;Studio apartment for double occupancy - £75 B&B There are both studio apartments with double and twin beds (limited number of twins). =Visitor Information= There will be a public lecture, [http://www.astro.ljmu.ac.uk/newsitem-20120315 First Light], given by Prof. James Dunlop on Tuesday 10th November 2015 at 18:00. [https://www.eventbrite.co.uk/e/astrophysics-first-light-prof-james-dunlop-tickets-18645744925 Click here to book free tickets]. General visitor information is available on the [http://www.visitliverpool.com/downtime Visiting Liverpool website]. <br>The city has several fine [http://www.liverpoolmuseums.org.uk/learning/contact.aspx Museums and Art Galleries] including a [http://www.liverpoolmuseums.org.uk/wml/visit/floor-plans/planetarium.aspx free planetarium]. 8c574a67483c6d29b6edcea59dc4cc22fe49096f 2084 2083 2015-10-19T15:20:46Z A.Piascik 40 /* Visitor Information */ Added pub map. Removed planetarium as too basic. wikitext text/x-wiki = Location Info = Place: Liverpool, UK Dates: 10-13 November 2015 Venue: Open Labs located in the IC1 building close to the [http://www.astro.ljmu.ac.uk/Main_Page Astrophysics Research Institute] &nbsp;&nbsp;[https://www.ljmu.ac.uk/contact-us/find-us/directions-jlad-and-im/open-labs-ic1-science-park IC1 Liverpool Science Park]<br> &nbsp;&nbsp;131 Mount Pleasant<br> &nbsp;&nbsp;Liverpool<br> &nbsp;&nbsp;L3 5TF<br> &nbsp;&nbsp;United Kingdom<br> &nbsp;&nbsp;+44 (0)151 705 3400<br> [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs [[File:gaia2015map1.png | pix 200]] ] The Gaia Workshop 2015 venue is marked in <font color="#db4436">red</font>. The Astrophysics Research Institute is on the 2^nd floor of the building marked in <font color="#3f5ba9">blue</font>. To view in more detail goto [https://www.google.com/maps/d/edit?mid=zVrgtauZeDS8.kzCze7erzmOs Google maps]. Streetview shown below as viewed from Mount Pleasant. Building is directly ahead. Access from Great Orford St: <html><iframe src="https://www.google.com/maps/embed?pb=!1m0!3m2!1sen!2sus!4v1438851417782!6m8!1m7!1s8hUVbU2RQmzQkahyi4xe2g!2m2!1d53.403649!2d-2.970505!3f53.27!4f1.9399999999999977!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> = Travel = == [[File:icon_plane.png | 32px | middle ]] Air Travel == These are a couple of useful flight search engines. *[http://www.momondo.co.uk/ momondo] *[http://www.skyscanner.net/ Sky Scanner] There are two airports providing access to the city of Liverpool. ==== LPL - Liverpool John Lennon Airport ==== * [http://www.liverpoolairport.com/ Liverpool John Lennon Airport] is located 14km from Liverpool city centre. [http://www.liverpoolairport.com/flight-information/airlines/ Airlines flying] to Liverpool airport are [http://www.easyjet.com/en/ easyJet], [http://www.ryanair.com/en/flights-to-liverpool/ RyanAir], [https://www.blueairweb.com/ Blue Air], [https://wizzair.com/en-GB/ Wizz Air], [http://www.czechairlines.com/ Czech Airlines], [https://flights.thomson.co.uk/ Thomson] and [http://www.aerlingus.com/en-gb/ Aer Lingus]. Although there is no rail link at the airport there are frequent bus services to [http://www.merseyrail.org/plan-your-journey/stations/liverpool-south-parkway.aspx Liverpool South Parkway] railway station, which is 10km from the city centre. <br>Liverpool South Parkway is a double railway station providing two separate rail routes into Liverpool Lime Street or Liverpool Central stations, which are in the city centre. After 9:30am a [http://www.merseytravel.gov.uk/Tickets/compare-tickets/Pages/Saveaway.aspx SaveAway] combined bus+train ticket can be purchased at the Information Desk on the lower level of the airport. <br>A SaveAway ticket including [http://www.merseytravel.gov.uk/Tickets/smartsaveaway/Pages/Area-Map.aspx Zones A,B,C & D] is suitable for a single journey to destinations in the city of Liverpool and costs £3.90. The [https://www.arrivabus.co.uk/north-west/journey-planner/ Arriva] bus services from the airport direct to Liverpool are [https://www.arrivabus.co.uk/north-west/services/500---liverpool-john-lennon-airport-to-liverpool/?direction=inbound 500], [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A], and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A], click on numbers to view routes and stops. These buses terminate at the [https://www.google.co.uk/maps/place/Liverpool+One+Bus+Station/@53.4017983,-2.9890373,17z/data=!3m1!4b1!4m2!3m1!1s0x487b212ecd2ebf57:0xb22b799b8e7f07c1 Liverpool One bus station]. <br>Services [https://www.arrivabus.co.uk/north-west/services/80-80a---liverpool-john-lennon-airport--speke-to-liverpool/?direction=inbound 80A] and [https://www.arrivabus.co.uk/north-west/services/86-86a-86d---liverpool-john-lennon-airport--garston-to-liverpool/?direction=inbound 86A] go via Liverpool South Parkway railway station if you wish to travel into Liverpool city by train. <br>The journey time into Liverpool by bus/train is approximately 25-45 minutes. A [http://www.liverpoolairport.com/airport-information/getting-to-from-the-airport/taxi/ taxi] to Liverpool city centre costs around £15.00 - £20.00 and takes approximately 20 minutes. ==== MAN - Manchester Airport ==== * [http://www.manchesterairport.co.uk/ Manchester Airport] is located 57km from Liverpool city centre. This airport is larger than Liverpool's so a greater number of [http://www.manchesterairport.co.uk/flight-information/flight-operators/ airlines] fly to this destination. The rail link at this airport is Manchester Airport [MIA] station. Trains operated by [http://www.northernrail.org/journey/planner Northern Rail] go direct to Liverpool Lime Street station every hour. [http://www.northernrail.org/pdfs/timetables/20150517/15.pdf Timetable]. <br>The journey time is approximately 1 hour. An alternative train route is from the airport station to Manchester Piccadilly [MAN] station and change there for trains to Liverpool Lime Street [LIV]. <br>Several train companies operate this alternative route. The journey time is approximately 1.5 hours. <br>Refer to [http://www.nationalrail.co.uk/ National Rail Enquiries] for train times. You can enter the three letter abbreviated [TLA] railway station IDs as shown. A taxi from Manchester airport to Liverpool city centre costs around £60. Journey is normally about 1 hour but will be longer if travelling during the rush hour. == [[File:icon_train.png | 32px | middle ]] Rail Travel == [http://www.nationalrail.co.uk/ National Rail Enquiries] is useful for planning rail travel with all UK train companies and for checking on delays or cancellations. <br>[http://www.thetrainline.com/farefinder/ The Trainline.com] is a search engine for finding low cost tickets. === In Liverpool === * [http://www.nationalrail.co.uk/stations_destinations/liv.aspx Liverpool Lime Street ] [LIV] is the main railway station destination located in the city. * Liverpool Central [LVC] station located in the city and is a local commuter destination for [http://www.merseyrail.org/ Merseyrail] trains. * Liverpool South Parkway [LPY] station is located 10km from the city and 4.5km from Liverpool John Lennon Airport. The railway system local to Liverpool is operated by [http://www.merseyrail.org/ Merseyrail]. The stations in and around the city can be view on [http://www.merseyrail.org/_common/map/networkmap.htm this map]. === From London === Trains to Liverpool Lime Street leave from [http://www.networkrail.co.uk/london-euston-station/departures-arrivals/ London Euston] [EUS]. There are a few trains direct but most require changing at Crewe [CRE] station. [http://www.virgintrains.co.uk/ Virgin Trains] operate the fastest service from London Euston to Liverpool Lime Street, the journey takes approximately 2.5 hours. Travelling [http://www.virgintrains.co.uk/assets/pdf/announcements/offpeak-and-superoffpeak-restrictions-2014.pdf Off-Peak] between 09:27 &rarr; 15:00 and after 18:45 is much cheaper. The cheapest [http://www.virgintrains.co.uk/tickets-offers/ticket-types/ tickets type] is Advance booking and can be purchased online up to 12 weeks prior to travel but are limited in availability and only valid for travel on the booked train. Tickets can be collected at the station but you must have the original credit/debit card used when purchasing. [http://tickets.londonmidland.com/lm/en/JourneyPlanning/MixingDeck London Midland Trains] operate a slower but cheaper train service. Travelling to Liverpool always requires a change of train at either Stafford [STA] or Crewe [CRE] and the journey time is approximately 3.5 hours. === Eurostar === [http://www.eurostar.com/ Eurostar] trains to the UK terminate at London [http://www.networkrail.co.uk/st-pancras-international-station/departures-arrivals/ St. Pancras International] [STP] which is 1km from London Euston where train to Liverpool Lime Street depart. <br>St. Pancras to Euston is a [https://www.google.co.uk/maps/dir/St+Pancras+International,+Euston+Rd,+London+N1C+4QP/Euston+Station,+London/@51.5291041,-0.1366104,16z/data=!4m13!4m12!1m5!1m1!1s0x48761b3b8d98ed25:0xb92d6fcfa832dd12!2m2!1d-0.126133!2d51.531427!1m5!1m1!1s0x48761b244f4bbe9b:0x9e50eedd53eb7ad8!2m2!1d-0.1321318!2d51.5279629 12 minute walk] or via the [https://tfl.gov.uk/cdn/static/cms/documents/standard-tube-map.pdf London Underground] on the <font color="#0583d2"><b>Victoria Line</b></font> or <b>Northern Line</b>. == [[File:icon_bus.png | 32px | middle ]] Bus Travel == [http://www.merseytravel.gov.uk/Pages/Welcome.aspx Merseytravel] has general information about public transport in Liverpool. <br>They provide a [http://jp.merseytravel.gov.uk/nwm/XSLT_TRIP_REQUEST2?language=en bus route planner] and a map of [http://www.merseytravel.gov.uk/travelling-around/key-destinations/Documents/LiverpoolPublicTransportMap.pdf Liverpool City Centre] bus routes. == [[File:icon_car.png | 32px | middle ]] Car Parking == [[File:gaia2015parking.png | 400px | left ]] There is no free street parking near the University and metered street parking, marked by blue and red lines, is expensive. Recommended parking close the venue is [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. This is a multi-story car park, marked <b><font color="red">P</font></b> on the map and is a [https://www.google.co.uk/maps/dir/38+Mt+Pleasant,+Liverpool,+Merseyside+L3+5TT/Liverpool+Science+Park,+131+Mount+Pleasant,+Liverpool+L3+5TF,+United+Kingdom/@53.4038119,-2.9745677,17z/data=!3m1!4b1!4m13!4m12!1m5!1m1!1s0x487b2123b1b6c19d:0x7752661a844802db!2m2!1d-2.9745775!2d53.4040468!1m5!1m1!1s0x487b211897cfef0b:0x325828a436916911!2m2!1d-2.9699337!2d53.4036712 5 minute walk] to the Gaia venue. All day parking costs £4, it is open from 7:00am until 20:00pm Mon-Fri, motorcycles and disabled are free. The entrance to the car park is at the lower end of Mount Pleasant, marked by the green dot on bottom of the £4 symbol. The car park has a one way system and the exit is onto Brownlow Hill. Full details are available from [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park]. The address is:- <br>&nbsp;&nbsp;38 Mount Pleasant <br>&nbsp;&nbsp;Liverpool <br>&nbsp;&nbsp;L3 5TB More information about parking in Liverpool is available from [http://en.parkopedia.co.uk/parking/liverpool/ Parkopedia]. <br clear="all"> =Accommodation= A large variety of hotels, hostels and B&Bs are available in Liverpool centre. Below are a selection of hotels that offer a discounted rate for the conference. There are generally 20 rooms reserved per large hotel (unless otherwise stated), most require telephone payments or payment on arrival. [http://www.daysinn.co.uk/hotels/united-kingdom/liverpool/days-inn-liverpool-city-centre/hotel-overview Days Inn Liverpool] The Days Inn hotel is located near the River Mersey and the Docks area (~5-10 minute walk) and from the city centre (<5 min walk). It is also next to James Street Station which can be directly accessed on the [http://www.merseyrail.org/ Mersey Rail Network] underground trains from Lime Street (a return or single from Lime Street to James Street costs less than £2). It is a ~20 minute walk from this hotel to the conference building. Parking is available nearby but isn’t cheap [http://www.q-park.co.uk/parking/parkingid/582 Q park]. To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are 20 rooms reserved at this rate from 9-13 November 2015 and will be available to book exclusively for the conference if booked before the end of September. After that the prices may be subject to change or rooms unavailable. Guests are able to book by calling 0151 203 1910 (option 1) Monday to Friday between 9am and 5pm or can email here reservations@daysinnliverpool.com. <br>&nbsp;&nbsp;£50 per night single occupancy (with Breakfast) <br>&nbsp;&nbsp;£60 per night double/twin occupancy (with Breakfast) [http://www.feathers.uk.com/feathers-hotel/ BEST WESTERN Feathers Liverpool Hotel] <br>0151 709 9655 <br>E-mail: [mailto:feathersreservations@feathers.uk.com feathersreservations@feathers.uk.com] The Feathers hotel is very close to the conference venue (~1 minute away). It is ~15 minute walk from Liverpool Lime Street station and from the centre of Liverpool. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). To book at this hotel please contact them directly and quote GAIA LIVERPOOL to receive this discounted rate. There are approximately 20 rooms being held for the conference. <br>&nbsp;&nbsp;Double for single occupancy: £69.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Double for double occupancy: £79.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for sole occupancy £84.95 (inc. breakfast and WiFi) <br>&nbsp;&nbsp;Exec double for double occupancy £89.95 (inc. breakfast and WiFi) [http://www.aachenhotel.co.uk/ Aachen Hotel], <br>89-91 Mount Pleasant <br>Liverpool <br>L3 5TB <br>T: +44 (0)151 709 3477 <br>T: +44 (0)151 709 3633 The Aachen Hotel is a small hotel on the same street as the conference venue (~5 min walk). There are no rooms reserved due to the size of the hotel but if you quote GAIA LIVERPOOL you can receive the discounted rate. Parking for this hotel is in the [http://liverpool.gov.uk/parking-travel-and-roads/council-car-parks/mount-pleasant/ Mount Pleasant Car Park] priced at £4 per day (see Transport Section). <br>&nbsp;&nbsp;£59 for a twin/double room [http://www.accorhotels.com/gb/hotel-7332-aparthotel-adagio-liverpool-city-centre/index.shtml Adagio Aparthotel Liverpool City Centre] <br>1 Fairclough Street <br>L1 1FS Liverpool <br>E-mail: [mailto:h7332-sl@adagio-city.com h7332-sl@adagio-city.com ] The Adagio Aparthotel is next to Liverpool Central Station (accessible via the Wirral line, one stop from Liverpool Lime street station). It is ~15 minute walk from here to the conference venue and the hotel is right in the middle of the city centre. Please contact the hotel directly via the email address above to book at these rates and quote GAIA LIVERPOOL. <br>&nbsp;&nbsp;Studio apartment for sole occupancy - £65 B&B <br>&nbsp;&nbsp;Studio apartment for double occupancy - £75 B&B There are both studio apartments with double and twin beds (limited number of twins). =Visitor Information= There will be a public lecture, [http://www.astro.ljmu.ac.uk/newsitem-20120315 First Light], given by Prof. James Dunlop on Tuesday 10th November 2015 at 18:00. [https://www.eventbrite.co.uk/e/astrophysics-first-light-prof-james-dunlop-tickets-18645744925 Click here to book free tickets]. General visitor information is available on the [http://www.visitliverpool.com/downtime Visiting Liverpool website]. <br>This site has a map of [http://www.visitliverpool.com/dbimgs/Real%20Ale%20Liverpool.pdf recommended pubs and inns] selling traditional beers and ales. The city has several fine [http://www.liverpoolmuseums.org.uk/learning/contact.aspx Museums and Art Galleries]. d282ed815f9e6b07048565e9bfb0669577e1a48d 0 256 2055 2008 2015-08-19T10:52:09Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett '''If you registered, but don't see your name here within a week, do email us!''' bb0fa86836788e6970e497f5571678acbb58f524 2056 2055 2015-08-19T14:29:47Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris '''If you registered, but don't see your name here within a week, do email us!''' 1e5549d25327d5664d3118b3cf6e886879255c07 2063 2056 2015-08-28T18:29:12Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila '''If you registered, but don't see your name here within a week, do email us!''' 6a8dda47c206571fc00779a386528a26e45a7697 2064 2063 2015-09-03T19:23:02Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn '''If you registered, but don't see your name here within a week, do email us!''' 60ecc32ab21c0745e763fb270ebc12cd3d58c399 2065 2064 2015-09-04T22:01:29Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell '''If you registered, but don't see your name here within a week, do email us!''' e27e4c9b19043cab53296817633188e149f6fe44 2067 2065 2015-09-10T11:00:28Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen '''If you registered, but don't see your name here within a week, do email us!''' 9b41c0a36153e069a55bc775e5c7b26f8c4172c1 2068 2067 2015-09-11T20:00:24Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore '''If you registered, but don't see your name here within a week, do email us!''' 0664f4b4d5bed1866b4d4fc896aa0c59c680c153 2069 2068 2015-09-18T15:24:00Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici '''If you registered, but don't see your name here within a week, do email us!''' 772d832033b96d0ac6c6947f1944b9e4cc51a821 2070 2069 2015-09-23T10:37:37Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams '''If you registered, but don't see your name here within a week, do email us!''' 17fb39c0facb8ef9168fe58bffa4e1adf1b8c58a 2071 2070 2015-09-29T08:57:43Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt '''If you registered, but don't see your name here within a week, do email us!''' 18c351cc5c0e520d1656d304a7a3cc55b8ae9edf 2072 2071 2015-10-03T20:52:54Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration will close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole '''If you registered, but don't see your name here within a week, do email us!''' 3b969108229d77adf6a0046b3348c6044f26d6fb 2073 2072 2015-10-05T14:59:57Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration extended until close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani '''If you registered, but don't see your name here within a week, do email us!''' a8cc13f98478aaf97653a192f9dce6dc08993f60 2074 2073 2015-10-07T20:03:42Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration extended until close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin '''If you registered, but don't see your name here within a week, do email us!''' 9019cc903223c8a59e42ebeecca4023700678986 2075 2074 2015-10-10T19:54:28Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration extended until close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova '''If you registered, but don't see your name here within a week, do email us!''' 2e204aad27963c6a29ef2b81703c10514c8ef63c 2076 2075 2015-10-12T12:23:55Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration extended until close '''30 September 2015''' <big>'''[http://www.astrouw.edu.pl/~wyrzykow/gaiaworkshop2015/registration.html REGISTER HERE]'''</big> Contact: gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki '''If you registered, but don't see your name here within a week, do email us!''' e044ed5ae07d320b72c0db894d262cdf28b30f0c 2077 2076 2015-10-12T12:24:39Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki '''If you registered, but don't see your name here within a week, do email us!''' 13b5712e894673a3e2d4c0d06d25d1533756c48a 2078 2077 2015-10-12T12:25:02Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki cd6a1ee4e2884ec450c7c14f13a7625efd2b84e2 2081 2078 2015-10-15T09:49:53Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell # Giuseppe Altavilla # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley # Pavel Koubsky # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk fda854f8b1ca000b452772fb0b21d3be67d0ba38 2085 2081 2015-10-26T19:44:28Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba 2e2e1a3f88f6fd639b12f52329c8d44aea8eaae3 2087 2085 2015-10-27T22:58:52Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane 19c5f34e2c0b05bcb6d06463c1bf565cf7a101de 2088 2087 2015-10-29T21:25:02Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane # Arancha Delgado 1d084b38814c2f74e6052e73b53015a15d2445d8 2101 2088 2015-11-02T13:42:53Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett # Manolis Xilouris # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane # Arancha Delgado # Grant Kennedy e8c3e2778f4446ec6817575623a9a7d93c52f5d3 0 255 2057 2011 2015-08-20T12:34:08Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2015.png|right|300px|Poster]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] REGISTRATION NOW OPEN! * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat 3bd8a345cd95334222765653856338acf36e3ca7 2060 2057 2015-08-20T12:35:54Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2015.png|right|300px]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] REGISTRATION NOW OPEN! * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat a83e4fdb242f72c6ec3dd8d309971f023f8611db 2061 2060 2015-08-20T12:36:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2015.png|right|450px]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants and Registration]] REGISTRATION NOW OPEN! * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat ddbd184e63d1d4a50a00865f387a7ccbfc0038c6 2082 2061 2015-10-19T11:54:05Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2015.png|right|450px]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants]] * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat 1d63f03911028225ecfcdb406d03c3ffa1e0cee0 6 265 2058 2015-08-20T12:34:30Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 266 2059 2015-08-20T12:35:27Z Gsawgwikiadmin 1 Created page with "[[Media:poster2015.png | Poster 2015 PNG format]]" wikitext text/x-wiki [[Media:poster2015.png | Poster 2015 PNG format]] aa74c5d2215b0c0e2926d942dfe3e0fba51eae8b 0 214 2066 1982 2015-09-04T22:02:37Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett # Fraser Lewis === GSAWG2: CVs and XRBs === This group has already established their own mailing list. Please contact the chair, Elme, if you want to join it. #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope #Fraser Lewis === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras #Fraser Lewis === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila #Fraser Lewis === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec #Fraser Lewis === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope #Fraser Lewis === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec #Fraser Lewis 20f463f96aa273cc66fe795853ba78622699b9d1 2086 2066 2015-10-26T21:52:58Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett # Fraser Lewis === GSAWG2: CVs and XRBs === This group has already established their own mailing list. Please contact the chair, Elme, if you want to join it. #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope #Fraser Lewis === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras #Fraser Lewis === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila #Fraser Lewis === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec #Fraser Lewis === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope #Fraser Lewis === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec #Fraser Lewis #Richard.Busuttil d255563b0af87fb90e1e58b78d09d2e03fc24c82 0 267 2089 2015-10-29T22:12:07Z Gsawgwikiadmin 1 Created page with "'''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>..." wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |} 8ecdb6ac41f62a00f68fea83437148e377ba01c7 2090 2089 2015-10-29T22:12:34Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |} 61714289459efb4dfb449d0c3a87b6190ddbf87a 2092 2090 2015-10-30T16:49:33Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all the speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} 803a81ee90d373479ca6c5f8c6c29425ce51045a 2093 2092 2015-10-30T16:52:32Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} fa1ccbf5e02e273b0f029f536ae0aa10a7293755 2094 2093 2015-10-30T17:04:31Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:Programme2015.pdf|Programme for printing]]</big> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} b74032f43c3a84a5cf1e2ce6899d1ee72f49e993 0 258 2091 2000 2015-10-29T22:13:29Z Gsawgwikiadmin 1 wikitext text/x-wiki We plan to start the meeting with lunch at 12:30 on Tuesday the 10th of November and finish with lunch on Friday 13th Nov. Detailed agenda will be composed of suggested contributions. Friday morning will probably be dedicated to the hands-on session and/or splinters. 0f272045632b3f64003c615aefd414585609fab1 2096 2091 2015-10-30T17:05:48Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:Programme2015.pdf|Programme for printing]]</big> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' fe923004248fc43696c57f7bf1e91d8157101078 2097 2096 2015-10-30T17:06:27Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:Programme2015.pdf Programme for printing]]</big> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 28afb2c95ff15d690efd6e75f0477da09459a0dc 2098 2097 2015-10-30T17:06:36Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[File:Programme2015.pdf|Programme for printing]]</big> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' fe923004248fc43696c57f7bf1e91d8157101078 2099 2098 2015-10-30T17:06:45Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <big>[[Media:Programme2015.pdf|Programme for printing]]</big> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 19393bfd5358f3e35a9c6e070b46a44dadb3af8f 2100 2099 2015-10-30T17:07:25Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |14:50 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:05 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:20 |'''coffee break''' | |0:40 |---- |16:00 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:15 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |16:35 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |16:55 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:10 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |'''discussion''' | |0:20 |---- |18:00 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |'''discussion''' | |0:30 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 4f0835a11ff9502916d4525792a596d17f91785a 6 268 2095 2015-10-30T17:04:48Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 258 2102 2100 2015-11-02T13:56:49Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |(TBC) |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS@ESO |0:15 |----- |16:50 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' a02d890d4edcfe2ea8a28fff36e5765e59bedcc7 2103 2102 2015-11-02T15:28:48Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS@ESO |0:15 |----- |16:50 |Manolis Xilouris |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 3b39ece7019e54b4002b0937c77f10d616ebe289 2105 2103 2015-11-02T21:56:31Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 61e3566da998af910aaaf4d7bce45efe7c32ebbc 2108 2105 2015-11-04T15:53:31Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 069a6cb6faafb2ec7e57e4037f0c14496e11d3a5 2109 2108 2015-11-04T15:58:06Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:50 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' ab6604e0e7df8dc4f5250200fb5a6c63a3267689 2110 2109 2015-11-05T15:46:15Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- |16:20 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:40 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |17:00 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:20 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:40 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |18:00 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 0204dcf71ef07a9455efcff0c0a354a8f4840a9c 2111 2110 2015-11-10T11:01:17Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- -> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' db385fbe84b6f1342faa3566bbe3c8fd35dce8a4 2112 2111 2015-11-10T11:01:30Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- -!> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 1960825420911057f0cd6adba055ad27ecf6e7d9 2113 2112 2015-11-10T11:01:46Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- --> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 0dcd9884eb315212fdd7a27f3b603bc7dc8b8827 2114 2113 2015-11-10T13:37:39Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- --> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |WORKSHOP PHOTO |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' b24359170867c9e781e45e134386df330fe1563c 2115 2114 2015-11-10T13:38:15Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book (draft)]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- --> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''WORKSHOP PHOTO''' |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 34f66e565099f47c0c5881a72c3ad34183f9779e 2117 2115 2015-11-10T17:21:03Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[File:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- --> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''WORKSHOP PHOTO''' |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' c1ebe40672bd0ea7175ee17d21ec412b987edaa2 2118 2117 2015-11-10T17:21:17Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- --> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''WORKSHOP PHOTO''' |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |'''discussion''' | |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Ulrich Kolb |PIRATE going forward |0:20 |---- |16:40 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:55 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |17:10 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:25 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:45 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |18:00 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |18:15 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 0197e43eb0fa01a1a5a5c67aa81db122fa2f3e98 2119 2118 2015-11-11T11:36:39Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- <!--|16:00 |Paul Groot |Gaia, BlackGEM and MeerLICHT: fast transients/variables |0:20 |---- --> |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''WORKSHOP PHOTO''' |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |16:50 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:05 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:55 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 8860c3c89e20dd5028ec470d3da9a292bddb5dd8 2120 2119 2015-11-11T12:59:15Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |'''WORKSHOP PHOTO''' |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |16:50 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:05 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:55 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 3f258de89ac607019e6675e3a4432665f2e0e922 2121 2120 2015-11-11T14:26:57Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg | WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Murat Dindar |TUG Software Tools for ToO Observations |0:15 |---- |16:50 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |17:05 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:25 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:40 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:55 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 7643a69840f5452272afbba40ee628b1efa3bc32 2124 2121 2015-11-11T14:31:07Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[File:GaiaWorkshop2015.jpg | WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' e635960db5e854f57912f3f37f7c85bf23d95de0 2125 2124 2015-11-11T14:31:29Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[File:GaiaWorkshop2015.jpg WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' b69c927d73a88d48c16793b13d71f97b70213189 2126 2125 2015-11-11T14:32:13Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' e6caf053f5e5e855bd340671350ca5d0b2302b59 2129 2126 2015-11-11T16:31:23Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |'''discussion''' | |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 7b7fb613dd3d5ffa6c86f7e3312059fda910b591 2130 2129 2015-11-11T23:23:16Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[File:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |'''discussion''' | |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' c09ee19f28ffd0579f2fd9d5fb08319ea8e52894 2131 2130 2015-11-11T23:23:29Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |'''discussion''' | |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 7b7fb613dd3d5ffa6c86f7e3312059fda910b591 2135 2131 2015-11-12T16:16:07Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts |0:30 |---- |10:30 |Heather Campbell |First science from Gaia |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes |0:20 |---- |17:30 |Giuseppe Leto |Catania participation in the Gaia Alerts Network |0:15 |---- |17:45 |Kris Rybicki |Loiano and Ostrowik Observatories |0:15 |---- |18:00 |Ulrich Kolb |PIRATE going forward |0:15 |---- |18:15 |'''discussion''' | |0:30 |---- |18:45 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE |0:20 |---- |15:10 |Gerry Gilmore |OPTICON |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy |0:15 |---- |17:40 |'''discussion''' | |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' d2373a4671ffbe7772528a366e17bf75715bd1fb 2136 2135 2015-11-25T09:39:11Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.pdf pdf] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.pdf pdf] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 0a6eda123aca91bccccf616e2ac1a3d1501c692e 2137 2136 2015-11-25T09:51:01Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] |0:20 |---- |17:40 |'''end of day 1''' | | |---- | | | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.pdf pdf] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.pdf pdf] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' b5be9b77347a539922c8c676c1063cd70f9b1cb1 2138 2137 2015-12-08T12:29:00Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BersierDavid.mov rec] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ReissDavid.mov rec] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/UlaczykKrzysztof.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/LewisFraser.mov rec] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BartletSophie.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartlettSophie.mov rec] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HourihaneAnna.mov rec] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/StaleyTim.mov rec] |0:20 |---- |17:40 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HodgkinSimon.mov rec] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_1.mov rec] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather1.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EyerLaurent.mov rec] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BlagorodnovaNadia.mov rec] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KennedyGrant.mov rec] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CopperwheatChris.mov rec] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BarnsleyRob.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/PiascikAndrzej.mov rec] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JermakHelen.mov rec] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/TurattoMassimo.mov rec] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BonanosAlceste.mov rec] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DamljanovicGoran.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.mov rec] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris1.mov rec] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KolbUlrich.mov rec] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionWed.mov rec] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JonkerPeter.mov rec] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/vanVelzenSjoert.mov rec] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WeversThomas.mov rec] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VerganiSusanna.mov rec] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/MattilaSeppo.mov rec] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/FraserMorgan.mov rec] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DellaValleMassimo.mov rec] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BreedtElme.mov rec] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris2.mov rec] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GilmoreGerry.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CarrascoJM.mov rec] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EreceOrhan.mov rec] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GodunovaVira.mov rec] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VotrubaViktor.mov rec] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WiersemaKlaas.mov rec] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ButkiewiczBakMagda.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.mov rec] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionThu.mov rec] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_2.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_3.mov rec] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather2.mov rec] |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 5c48d92c7537c4aa8eba208d7b7ed496cffc3131 2139 2138 2015-12-08T12:30:34Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BersierDavid.mov rec] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ReissDavid.mov rec] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/UlaczykKrzysztof.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/LewisFraser.mov rec] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BartlettSophie.mov rec] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HourihaneAnna.mov rec] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/StaleyTim.mov rec] |0:20 |---- |17:40 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HodgkinSimon.mov rec] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_1.mov rec] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather1.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EyerLaurent.mov rec] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BlagorodnovaNadia.mov rec] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KennedyGrant.mov rec] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CopperwheatChris.mov rec] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BarnsleyRob.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/PiascikAndrzej.mov rec] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JermakHelen.mov rec] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/TurattoMassimo.mov rec] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BonanosAlceste.mov rec] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DamljanovicGoran.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.mov rec] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris1.mov rec] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KolbUlrich.mov rec] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionWed.mov rec] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JonkerPeter.mov rec] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/vanVelzenSjoert.mov rec] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WeversThomas.mov rec] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VerganiSusanna.mov rec] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/MattilaSeppo.mov rec] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/FraserMorgan.mov rec] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DellaValleMassimo.mov rec] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BreedtElme.mov rec] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris2.mov rec] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GilmoreGerry.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CarrascoJM.mov rec] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EreceOrhan.mov rec] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GodunovaVira.mov rec] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VotrubaViktor.mov rec] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WiersemaKlaas.mov rec] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ButkiewiczBakMagda.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.mov rec] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionThu.mov rec] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_2.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_3.mov rec] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather2.mov rec] |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 31d74c87200b9d34859e95d3d749f14c69564cc8 2140 2139 2015-12-08T12:34:35Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BersierDavid.mov rec] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ReissDavid.mov rec] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/UlaczykKrzysztof.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/LewisFraser.mov rec] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BartlettSophie.mov rec] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HourihaneAnna.mov rec] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/StaleyTim.mov rec] |0:20 |---- |17:40 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HodgkinSimon.mov rec] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_1.mov rec] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather1.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EyerLaurent.mov rec] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BlagorodnovaNadia.mov rec] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KennedyGrant.mov rec] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CopperwheatChris.mov rec] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BarnsleyRob.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/PiascikAndrzej.mov rec] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JermakHelen.mov rec] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/TurattoMassimo.mov rec] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BonanosAlceste.mov rec] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DamljanovicGoran.mov rec] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris1.mov rec] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KolbUlrich.mov rec] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionWed.mov rec] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JonkerPeter.mov rec] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/vanVelzenSjoert.mov rec] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WeversThomas.mov rec] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VerganiSusanna.mov rec] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/MattilaSeppo.mov rec] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/FraserMorgan.mov rec] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DellaValleMassimo.mov rec] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BreedtElme.mov rec] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris2.mov rec] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GilmoreGerry.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CarrascoJM.mov rec] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EreceOrhan.mov rec] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GodunovaVira.mov rec] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VotrubaViktor.mov rec] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WiersemaKlaas.mov rec] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ButkiewiczBakMagda.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.mov rec] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionThu.mov rec] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_2.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_3.mov rec] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather2.mov rec] |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 8149158bea7ca2271fb05bff7b687c28ead4105b 2141 2140 2015-12-08T12:38:22Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BersierDavid.mov rec] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ReissDavid.mov rec] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/UlaczykKrzysztof.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/LewisFraser.mov rec] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BartlettSophie.mov rec] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HourihaneAnna.mov rec] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/StaleyTim.mov rec] |0:20 |---- |17:40 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HodgkinSimon.mov rec] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_1.mov rec] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather1.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EyerLaurent.mov rec] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BlagorodnovaNadia.mov rec] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KennedyGrant.mov rec] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CopperwheatChris.mov rec] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BarnsleyRob.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/PiascikAndrzej.mov rec] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JermakHelen.mov rec] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/TurattoMassimo.mov rec] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BonanosAlceste.mov rec] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DamljanovicGoran.mov rec] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris1.mov rec] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KolbUlrich.mov rec] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionWed.mov rec] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JonkerPeter.mov rec] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/vanVelzenSjoert.mov rec] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WeversThomas.mov rec] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VerganiSusanna.mov rec] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/MattilaSeppo.mov rec] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/FraserMorgan.mov rec] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DellaValleMassimo.mov rec] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BreedtElme.mov rec] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris2.mov rec] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GilmoreGerry.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CarrascoJM.mov rec] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EreceOrhan.mov rec] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GodunovaVira.mov rec] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VotrubaViktor.mov rec] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WiersemaKlaas.mov rec] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ButkiewiczBakMagda.mov rec] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionThu.mov rec] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_2.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_3.mov rec] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather2.mov rec] |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 5144ae663b774b326663813350c7bd752802686a 2142 2141 2015-12-08T14:30:51Z Gsawgwikiadmin 1 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BersierDavid.mov rec] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ReissDavid.mov rec] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/UlaczykKrzysztof.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/LewisFraser.mov rec] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BartlettSophie.mov rec] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HourihaneAnna.mov rec] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/StaleyTim.mov rec] |0:20 |---- |17:40 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HodgkinSimon.mov rec] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_1.mov rec] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather1.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EyerLaurent.mov rec] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BlagorodnovaNadia.mov rec] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KennedyGrant.mov rec] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CopperwheatChris.mov rec] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BarnsleyRob.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/PiascikAndrzej.mov rec] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JermakHelen.mov rec] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/TurattoMassimo.mov rec] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BonanosAlceste.mov rec] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DamljanovicGoran.mov rec] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris1.mov rec] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionWed.mov rec] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JonkerPeter.mov rec] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/vanVelzenSjoert.mov rec] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WeversThomas.mov rec] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VerganiSusanna.mov rec] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/MattilaSeppo.mov rec] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/FraserMorgan.mov rec] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DellaValleMassimo.mov rec] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BreedtElme.mov rec] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris2.mov rec] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GilmoreGerry.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CarrascoJM.mov rec] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EreceOrhan.mov rec] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GodunovaVira.mov rec] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VotrubaViktor.mov rec] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WiersemaKlaas.mov rec] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ButkiewiczBakMagda.mov rec] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionThu.mov rec] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_2.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_3.mov rec] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather2.mov rec] |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' 350fb59dd73b470854af8e0d312e9662dc716928 2143 2142 2015-12-09T11:09:14Z Zuzanna 36 wikitext text/x-wiki '''<big>To all speakers: please send your slides prior to your presentation to Lukasz Wyrzykowski. Accepted formats: PDF, Keynote, PowerPoint, OpenOffice</big>''' <!--<big>[[Media:Programme2015.pdf|Programme for printing]]</big>--> <big>[[Media:AbstractBook2015.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- | | | | |---- |colspan="4"|'''Tuesday, 10 November 2015''' |---- |10:00 |'''registration desk open''' | | |---- |12:30 |'''lunch''' | |1:30 |---- |14:00 | |Welcome |0:10 |---- |14:10 |David Bersier |ASAS-SN: The All-Sky Automated Survey for SuperNovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BersierDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BersierDavid.mov rec] |0:20 |---- |14:30 |David Reiss |LSST Transient Alert Production Pipeline [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ReissDavid.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ReissDavid.mov rec] |0:20 |---- |14:50 |Zuzanna Kostrzewa-Rutkowska |OGLE-IV Transient Survey [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KostrzewaRutkowskaZuzanna.pdf pdf] |0:20 |---- |15:10 |Krzysztof Ulaczyk |The Gravitational-wave Optical Transient Observer [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/UlaczykKrzysztof.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/UlaczykKrzysztof.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Fraser Lewis |Education and Outreach Opportunities from Gaia Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/LewisFraser.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/LewisFraser.mov rec] |0:20 |---- |16:20 |Sophie Bartlett |Getting to know Gaia - Applying a current, real-world context to the school science curriculum [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BartletSophie.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BartlettSophie.mov rec] |0:20 |---- |16:40 |Anna Hourihane |Gaia Science Alerts for outreach: publication and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HourihaneAnna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HourihaneAnna.mov rec] |0:20 |----- |17:00 |Lorraine Hanlon <!-- NO VIDEO PLEASE --> |Watcher robotic telescope and Gaia archive [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HanlonLorraine.pdf pdf] |0:20 |---- |17:20 |Tim Staley |Beyond ATEL's - How to hook in to the VOEvent network [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/StaleyTim.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/StaleyTim.mov rec] |0:20 |---- |17:40 |'''end of day 1''' | | |---- |colspan="4"|'''Wednesday, 11 November 2015''' |---- |09:30 |Simon Hodgkin |Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/HodgkinSimon.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/HodgkinSimon.mov rec] |0:30 |---- |10:00 |Lukasz Wyrzykowski |First year of the Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_1.mov rec] |0:30 |---- |10:30 |Heather Campbell |First science from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CampbellHeather.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather1.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Laurent Eyer |Variable stars in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EyerLaurent.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EyerLaurent.mov rec] |0:25 |---- |12:10 |Nic Walton |Gaia Science Alerts in the Main Gaia Data Releases [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WaltonNic.pdf pdf] <!-- DO NOT ADD VIDEO --> |0:20 |---- |12:30 |Nadejda Blagorodnova |Nuclear transient detection with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BlagorodnovaNadia.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BlagorodnovaNadia.mov rec] |0:30 |---- |13:00 |[[Media:GaiaWorkshop2015.jpg|WORKSHOP PHOTO]] |''steps to the Cathedral'' | |---- |13:10 |'''lunch break''' | |1:30 |---- |14:30 |Grant Kennedy |Transits of exploding asteroids and fragmented comets [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KennedyGrant.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/KennedyGrant.mov rec] |0:20 |---- |14:50 |Chris Copperwheat |Gaia transients with the Liverpool Telescope and Liverpool Telescope 2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CopperwheatChris.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CopperwheatChris.mov rec] |0:20 |---- |15:10 |Rob Barnsley |IO:I - a new infrared imager for the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BarnsleyRob.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BarnsleyRob.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Andrzej Piascik |Spectrographic Classification of Transients with the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/PiascikAndrzej.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/PiascikAndrzej.mov rec] |0:20 |---- |16:20 |Helen Jermak |LOTUS: a low-cost UV spectrograph on the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JermakHelen.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JermakHelen.mov rec] |0:15 |---- |16:35 |Massimo Turatto |SOXS, the next generation instrument for ESO NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/TurattoMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/TurattoMassimo.mov rec] |0:15 |----- |16:50 |Alceste Bonanos |Observing facilities at the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BonanosAlceste.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/BonanosAlceste.mov rec] |0:20 |---- |17:10 |Goran Damljanovic |Gaia-FUN-TO and the observations of Gaia Alerts objects using Serbian-Bulgarian mini-network telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DamljanovicGoran.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DamljanovicGoran.mov rec] |0:20 |---- |17:30 |Kris Rybicki |Loiano and Ostrowik Observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris1.mov rec] |0:15 |---- |17:45 |Ulrich Kolb |PIRATE going forward [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/KolbUlrich.pdf pdf] |0:15 |---- |18:00 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsWed.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionWed.mov rec] |0:30 |---- |18:30 |''end of day 2'' | | |---- |19:30 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Thursday, 12 November 2015''' |---- |09:30 |Peter Jonker |TDEs with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/JonkerPeter.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/JonkerPeter.mov rec] |0:25 |---- |09:55 |Sjoert van Velzen |Optical observations of stellar tidal disruption flares [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/vanVelzenSjoert.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/vanVelzenSjoert.mov rec] |0:25 |---- |10:20 |Thomas Wevers |Fast transients from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WeversThomas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WeversThomas.mov rec] |0:20 |---- |10:40 |Susanna Vergani |Catching GRB orphan afterglows from Gaia triggers [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VerganiSusanna.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VerganiSusanna.mov rec] |0:20 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Seppo Mattila |Nuclear supernovae with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/MattilaSeppo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/MattilaSeppo.mov rec] |0:25 |---- |12:10 |Morgan Fraser |Freaks and weirdos - A taxonomy of rare, peculiar and puzzling supernovae [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/FraserMorgan1.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/FraserMorgan.mov rec] |0:25 |---- |12:35 |Massimo Della Valle |Novae in the Gaia Era [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DellaValleMassimo.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/DellaValleMassimo.mov rec] |0:25 |---- |13:00 |'''lunch break''' | |1:30 |---- |14:30 |Elme Breedt |Accreting compact object binaries from Gaia and other transient surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/BreedtElme.pdf pdf] |0:20 |---- |14:50 |Kris Rybicki |Astrometric microlensing from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/RybickiKris2.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/RybickiKris2.mov rec] |0:20 |---- |15:10 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GilmoreGerry.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GilmoreGerry.mov rec] |0:15 |---- |15:25 |'''coffee break''' | |0:35 |---- |16:00 |Josep Manel Carrasco |The Montsec Observatory and the Gaia science alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/CarrascoJosep.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CarrascoJM.mov rec] |0:20 |---- |16:20 |Orhan Erece |Observations, Contributions and A New Follow-Up Software at TUG [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/EreceOrhan.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/EreceOrhan.mov rec] |0:15 |---- |16:35 |Vira Godunova |Monitoring of transient phenomena at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/GodunovaVira.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/GodunovaVira.mov rec] |0:15 |---- |16:50 |Viktor Votruba |Danish 1.54m telescope na La Silla and Czech participation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/VotrubaViktor.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/VotrubaViktor.mov rec] |0:20 |---- |17:10 |Klaas Wiersema |Observing transients with the University of Leicester observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WiersemaKlaas.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WiersemaKlaas.mov rec] |0:15 |---- |17:25 |Magda Butkiewicz-Bąk |Global Astrophysical Telescope System - a new tool for photometry and spectroscopy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/ButkiewiczBakMagda.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/ButkiewiczBakMagda.mov rec] |0:15 |---- |17:40 |'''discussion''' | [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/discussionsThu.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/discussionThu.mov rec] |0:30 |---- |18:10 |''end of day 3'' | | |---- |---- |colspan="4"|'''Friday, 13 November 2015''' |---- |09:30 |Arancha Delgado |Introduction to the new Gaia Alerts Interface [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/DelgadoArancha.pdf pdf] |0:30 |---- |10:00 |Morgan Fraser |Running a successful spectroscopic programme - lessons from PESSTO |0:30 |---- |10:30 |Lukasz Wyrzykowski |How to do the photometric follow-up? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-Follow-up.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_2.mov rec] |0:30 |---- |11:00 |'''coffee break''' | |0:45 |---- |11:45 |Lukasz Wyrzykowski |Introduction to the Calibration Server and other tools [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/slides/WyrzykowskiLukasz-CalibrationServer.pdf pdf] [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/WyrzykowskiLukasz_3.mov rec] |0:30 |---- |12:15 |Heather Campbell |Photometric classification of transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2015/movies/CampbellHeather2.mov rec] |0:30 |---- |12:45 |'''lunch and end of the meeting''' | | |---- |} '''NOTE: agenda might still change slightly''' b5e5089fd03e6920a74cafd944b7cfa574e96286 0 256 2104 2101 2015-11-02T21:54:55Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett <!--# Manolis Xilouris--> # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane # Arancha Delgado # Grant Kennedy # Alceste Bonanos 74e577bb0bdf10d655bf0aa1cbf7996f54340918 2106 2104 2015-11-04T13:49:23Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett <!--# Manolis Xilouris--> # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane # Arancha Delgado # Grant Kennedy # Alceste Bonanos # Gavin Lamb 7cf72f58d362f6a6ba6b99596986870842501384 2107 2106 2015-11-04T13:51:27Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett <!--# Manolis Xilouris--> # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane # Arancha Delgado # Grant Kennedy # Alceste Bonanos # Gavin Lamb # Harry Brown 83b1c9008ce6fe23b8c8c35ff8b3a559e6d0e69c 2133 2107 2015-11-12T01:00:08Z Gsawgwikiadmin 1 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration is now closed. But if you are still desperate to come, drop us an email at gaiasciencealertsworkshop2015@gmail.com === List of registered participants === # Sheila McBreen # Derek O'Callaghan # Łukasz Wyrzykowski # Morgan Fraser # Mike Bode # Paul Groot # Tim Staley # Giuseppe Leto # Matt Darnley # Murat Dindar # Murat Parmaksizoglu # Peter Jonker # Ulrich Kolb # Goran Damljanovic # Klaas Wiersema # Nicholas Walton # Josep Manel Carrasco # Patricia Whitelock # Fraser Lewis # Sophie Bartlett <!--# Manolis Xilouris--> # Armin Rasekh # Seppo Mattila # David Lynn # Carole Mundell # Iain Steele # Chris Copperwheat # Goska van Leeuwen # Martin Dominik # Gerry Gilmore # Thomas Wevers # Andreja Gomboc # Lorraine Hanlon # Aurora Clerici # David Bersier # Drejc Kopac # Steven Williams # Johanna F Jarvis # Heather Campbell <!-- # Giuseppe Altavilla--> # Krzysztof Ulaczyk # Orhan Erece # Francesca Onori # Tuomas Kangas # David Reiss # Elme Breedt # Massimo Turatto # Helen Jermak # Vira Godunova # Rob Barnsley <!-- # Pavel Koubsky--> # George Seabroke # Sjoert van Velzen # Mohamed Nabil Bendris # Robin Catchpole # Andrzej Piascik # Susanna Vergani # Massimo Della Valle # Laurent Eyer # Simon Hodgkin # Philip James # Nadejda Blagorodnova Mujortova # Zuzanna Kostrzewa-Rutkowska # Kris Rybicki # Shiho Kobayashi # Magda Butkiewicz-Bąk # Viktor Votruba # Anna Hourihane # Arancha Delgado # Grant Kennedy # Alceste Bonanos # Gavin Lamb # Harry Brown # MIchal Ciszek 99e030b0f6cce5096755347b1f488865fe6785fc 6 269 2116 2015-11-10T17:12:59Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 270 2122 2015-11-11T14:27:15Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2123 2122 2015-11-11T14:29:35Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:GaiaWorkshop2015.jpg]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2132 2123 2015-11-11T23:25:10Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:GaiaWorkshop2015.jpg]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 255 2127 2082 2015-11-11T15:13:47Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2015.png|right|450px]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants]] * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg]] 5992bb2a886f60e455231620e03a1a8b315e366a 2128 2127 2015-11-11T15:14:42Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2015.png|right|450px]] '''The sixth Gaia Science Alerts workshop will be held in [[Workshop2015:logistics | Liverpool on 10-13 November 2015]].''' The topics this year include: * Status of Gaia * First year of Gaia Alerts * Results from the Verification Phase * Gaia alerts follow-up campaigns * Science with Gaia transients: Supernovae, Microlensing, Novae, TDEs, CVs, YSOs * Current/planned multi-wavelength transient surveys and synergy * Training in follow-up tools for Gaia Alerts ---- * [[workshop2015:rationale|Rationale]] * [[workshop2015:agenda|Agenda]] * [[workshop2015:registration|Participants]] * [[workshop2015:logistics|Logistic information]] * [[workshop2015:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === * Lukasz Wyrzykowski * Iain Steele * Simon Hodgkin * Zuzanna Kostrzewa-Rutkowska LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] c13902cbc8ef21489afb12a162ec16c2a7381f2c 0 214 2134 2086 2015-11-12T13:15:52Z Gsawgwikiadmin 1 /* GSAWG5: AGNs and TDEs */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett # Fraser Lewis === GSAWG2: CVs and XRBs === This group has already established their own mailing list. Please contact the chair, Elme, if you want to join it. #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope #Fraser Lewis === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras #Fraser Lewis === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila #Fraser Lewis === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] #Sheila McBreen #David Lynn #Derek O'Callaghan === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec #Fraser Lewis === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope #Fraser Lewis === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec #Fraser Lewis #Richard.Busuttil 63d77ceb258184d66a5bfd1ce1804ffd88eea87b 2144 2134 2016-02-06T11:54:10Z Sth 6 /* GSAWG10: Photometric Follow-Up */ wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett # Fraser Lewis === GSAWG2: CVs and XRBs === This group has already established their own mailing list. Please contact the chair, Elme, if you want to join it. #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope #Fraser Lewis === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras #Fraser Lewis === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila #Fraser Lewis === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] #Sheila McBreen #David Lynn #Derek O'Callaghan === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec #Fraser Lewis === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope #Fraser Lewis === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec #Fraser Lewis #Richard.Busuttil #Simon Hodgkin 80066aa359062005102ffb55464d7765c08b8492 0 17 2145 1998 2016-07-05T07:43:07Z Lukasz 2 wikitext text/x-wiki == Gaia Science Alerts Follow-up Server == We are currently testing a facility which allows uniform calibration of the photometric follow-up observations of alerts reported by transient surveys. <big> Access to the Calibration Server: [http://gsaweb.ast.cam.ac.uk/followup/]. Here is the presentation about it: [[Media:GaiaFollowupServerManual.pdf | Presentation]] Here is the documentation on the [[Calibration_Server|Cambridge Photometry Calibration Server]] </big> If you plan to perform any photometric follow-up observations of the alerts available at SkyAlert.org and you would like to use our service, please contact [[User:Lukasz | Lukasz Wyrzykowski]] for password. When contacting us please provide us also with your observatory name, longitude and latitude and available filters. Useful links for observers willing to do follow-up observations for Gaia: * [http://nova.astrometry.net astrometry.net] - online service providing astrometric WCS solution for any image * [http://www.astromatic.net astromatic.net] - collection of useful astro-software, including Sextractor == Preliminary minimal requirements on the photometric and spectroscopic follow-up of Gaia Alerts == '''Photometry:''' * multi-band photometry, at least two bands (e.g. V,I), Sloan ugriz preferred * flux calibration no worse than 10% (0.1 mag) * WCS and fluxes (from, e.g., Sextractor) submitted to the Calibration Server * availability of flux measurements within 24 hours '''Spectroscopy:''' * spectral range minimal: 4500-7000A * signal to noise > 20 all over the range above * resolution R > 150 * lambda calibrations better -+ 3A * relative flux calibrations better -+10% * absolute flux calibrations: none * availability of reduced spectra within less than 24h == Coordination of follow-up spectroscopy and photometry == There is a new page discussing strategy, schedules, observing rotas and an observing guide: [[ObservingProgramme | here]] == GAIA Marshall == The GAIA Marshall can be found at: http://gaiamarshall.ast.cam.ac.uk Username and password are required to access the GAIA Marshall facility. =====Catalogues Cross-matched and Update Frequencies ===== * GAIA Alerts: Every 1 hour * ASAS - SN: Every 3 hours * CRTS - CV (CSS, MSL and SSS): Every 3 hours * CRTS - SN (CSS, MSL and SSS): Every 3 hours * OGLE: Every 1 hour * Pan-STARRS: Every 3 hours * SkyMapper: Every 3 hours * Sources added by users: Every 3 hours * ATelegrams: Every 1 hour =====Marshall How-to and Known Bugs===== * [[marshall how-to]] * [[File: Gaia_marshall_tutorial.pdf]] * [[Marshall known bugs]] 9b52c82797e6809767b7bd82f5c09b2e2337750c 0 1 2146 2009 2016-08-31T13:16:30Z Lukasz 2 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2016:main|7th Gaia Science Alerts Workshop 2016, Utrecht]]</Big>''' </center> ---- <center> [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 9fa926ecc12419bea5db1754404dd1ea86656817 0 271 2147 2016-08-31T13:16:48Z Lukasz 2 Created page with "Utrecht, 7-9 December 2016." wikitext text/x-wiki Utrecht, 7-9 December 2016. 73e33207c3cb2723d921b43eb9129ad591fd01d0 2148 2147 2016-09-05T12:04:53Z Lukasz 2 wikitext text/x-wiki Utrecht or Nijmegen, NL, 7-9 December 2016. d74bdf6426b54d7b96f10eaf0889a1ff6a0b00a5 2149 2148 2016-09-06T08:50:01Z Zuzanna 36 wikitext text/x-wiki Utrecht or Nijmegen, NL, 7-9 December 2016. * [[workshop2016:registration|Registration]] 090ff0661856160d98360a89c4d79ce3c06162c5 0 272 2150 2016-09-09T09:11:13Z Zuzanna 36 Created page with "Pre-registration form: [https://goo.gl/forms/xWY98Negxx0eiz8a2 link]" wikitext text/x-wiki Pre-registration form: [https://goo.gl/forms/xWY98Negxx0eiz8a2 link] 1947f80db9dfec9fe074c057788a405c1ee6d850 2151 2150 2016-09-09T09:19:19Z Zuzanna 36 wikitext text/x-wiki Pre-registration form: [https://goo.gl/forms/xWY98Negxx0eiz8a2 link] We confirm your registration by e-mail in November. fe70fee9acc72ea522f8fc31cc13f5f3a55a79ea 8 3 2152 1987 2016-09-12T13:55:39Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2016 **workshop2016:main|Main Workshop Page **workshop2016:rationale|Rationale **workshop2016:agenda|Program **workshop2016:registration|Participants and Registration **workshop2016:logistics|Logistics *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 614b00cf575b9f84c260fe8ce9f3fb257a984b61 0 273 2153 2016-09-12T13:59:44Z Gsawgwikiadmin 1 Created page with "Gaia has been operating already for two and a half years. Hundreds of billions of observations have been collected and with the first Gaia Data Release in September, Gaia is i..." wikitext text/x-wiki Gaia has been operating already for two and a half years. Hundreds of billions of observations have been collected and with the first Gaia Data Release in September, Gaia is initiating a revolution in astronomy in general and in our understanding of the Milky Way in particular. In addition, nearly 1000 alerts have been issued by the Gaia Science Alerts group. Gaia is now the second largest provider of transients in the world! Many of the alerts has been intensively followed-up by multiple observatories, with interesting discoveries of rare types of supernovae, cataclysmic variables, microlensing events and other exotic transients. This December we would like to gather again for the 7th Gaia Science Alerts Workshop at SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. The aims of this workshop are the following: - present and discuss scientific results from the Gaia Alerts so far - discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) - discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts - present the status and the organisation of the H2020 OPTICON follow-up network - receive feedback from the users to Gaia Alerts - discuss and recognise future steps in improving the follow-up programmes abbbf4d28dc32c674f21f1f4d855cdec7e118366 2162 2153 2016-09-12T14:37:47Z Gsawgwikiadmin 1 wikitext text/x-wiki Gaia has been operating already for two and a half years. Hundreds of billions of observations have been collected and with the first Gaia Data Release in September, Gaia is initiating a revolution in astronomy in general and in our understanding of the Milky Way in particular. In addition, nearly 1000 alerts have been issued by the Gaia Science Alerts group. Gaia is now the second largest provider of transients in the world! Many of the alerts has been intensively followed-up by multiple observatories, with interesting discoveries of rare types of supernovae, cataclysmic variables, microlensing events and other exotic transients. This December we would like to gather again for the 7th Gaia Science Alerts Workshop at SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. The aims of this workshop are the following: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes cdacbc449114beb64f131989d83c9dfe1517a0d6 0 274 2154 2016-09-12T14:00:57Z Gsawgwikiadmin 1 Created page with "We plan to start on Wed 7.Dec in the morning and finish by lunch time on Friday." wikitext text/x-wiki We plan to start on Wed 7.Dec in the morning and finish by lunch time on Friday. de2d929bf664aa66cebcbb566951e80745a7199b 2185 2154 2016-11-17T23:00:32Z Gsawgwikiadmin 1 wikitext text/x-wiki We plan to start on Wed 7.Dec in the morning and finish by lunch time on Friday. '''AGENDA coming here soon.''' On Friday morning we plan to have a hands-on session on data reduction procedures and usage of the Calibration Server. 4215fae9961b8d4db943118b88de69c88c56bbc0 2186 2185 2016-11-17T23:00:57Z Gsawgwikiadmin 1 wikitext text/x-wiki We plan to start on Wed 7.Dec with lunch and finish by lunch time on Friday. '''AGENDA coming here soon.''' On Friday morning we plan to have a hands-on session on data reduction procedures and usage of the Calibration Server. f7a678818503df5ea22e47d909b05915ff87e48a 2187 2186 2016-11-25T11:32:41Z Zuzanna 36 wikitext text/x-wiki {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |09:55 |Peter Jonker |Nuclear transients |0:25 |---- |10:20 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |10:40 |'''coffee break''' | |0:40 |---- |11:20 |Thomas Wevers |TBA |0:25 |---- |11:45 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |12:05 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:25 |'''lunch''' | |1:35 |---- |14:00 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:25 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |14:50 |Gerry Gilmore |OPTICON |0:15 |---- |15:05 |Andreja Gomboc |TBC |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:15 |---- |16:50 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:05 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:45 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 2e7e007a0fdef124b54477e74b8485c68c1fd855 2188 2187 2016-11-25T11:35:58Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |09:55 |Peter Jonker |Nuclear transients |0:25 |---- |10:20 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |10:40 |'''coffee break''' | |0:40 |---- |11:20 |Thomas Wevers |TBA |0:25 |---- |11:45 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |12:05 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:25 |'''lunch''' | |1:35 |---- |14:00 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:25 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |14:50 |Gerry Gilmore |OPTICON |0:15 |---- |15:05 |Andreja Gomboc |TBC |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:15 |---- |16:50 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:05 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:45 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:45 |'''lunch''' | |1:15 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' eb700083fcd470bcd5fdae2c7fa06a32179a7774 2189 2188 2016-11-25T13:35:12Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |09:55 |Peter Jonker |Nuclear transients |0:25 |---- |10:20 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |10:40 |'''coffee break''' | |0:40 |---- |11:20 |Thomas Wevers |TBA |0:25 |---- |11:45 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |12:05 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:25 |'''lunch''' | |1:35 |---- |14:00 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:25 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |14:50 |Gerry Gilmore |OPTICON |0:15 |---- |15:05 |Andreja Gomboc |TBC |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:15 |---- |16:50 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:05 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:45 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 55b228ea6080e6822b82bcd072f0185a4af33023 2192 2189 2016-11-30T21:28:17Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |TBA |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Andreja Gomboc |TBC |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:15 |---- |16:50 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:05 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:45 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 480a42e5e36604f0adf4e51cd5974dbf8d98340a 2193 2192 2016-12-01T10:36:17Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Andreja Gomboc |TBC |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:15 |---- |16:50 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:05 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:45 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' c8a5fe8636c837c81e98345a556b276b591f6a7d 2194 2193 2016-12-01T16:09:04Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:15 |---- |16:50 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:05 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:45 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |TBC |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' b219c971ed6d5a74b6f9c31e2462ab82d9d34620 2195 2194 2016-12-05T11:50:55Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |TBC |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' b546e62b8044c83f8dde60283462110df394d6d1 2196 2195 2016-12-06T21:02:25Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 66a11cf1ee61201ed661c9b5ada2225de59ec752 2197 2196 2016-12-07T11:04:55Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' <big>[[File:abstractbook2016.pdf|Abstract book]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 27c36d6a55ebbd2c54fdba81a17e3d54f2933280 2199 2197 2016-12-07T11:07:38Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' <big>[[File:abstractbook2016.pdf|Abstract book]]</big> <big>[[Media:abstractbook2016.pdf|Abstract book and agenda [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 214a7d469ec94ebe67b60c5dc0a23c0fa8f363cc 2200 2199 2016-12-07T11:08:03Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' <big>[[Media:abstractbook2016.pdf|Abstract book [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope |0:20 |---- |10:50 |Alireza Molaeinezhad |TBA |0:15 |---- |11:05 |'''coffee break''' | |0:30 |---- |11:35 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 11dc969c8f21c58edba11184cded38275c9817b6 2201 2200 2016-12-08T09:12:44Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' <big>[[Media:abstractbook2016.pdf|Abstract book [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''coffee break''' | |0:40 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope |0:20 |---- |10:50 |'''coffee break''' | |0:30 |---- |11:20 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:20 | |Closing remarks |0:15 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' be52c2473dd5cb0269841710fe2f85fe54b014f1 0 275 2155 2016-09-12T14:02:19Z Gsawgwikiadmin 1 Created page with "The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. More information on the logistics will be provided here soon." wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. More information on the logistics will be provided here soon. 0fdcce74d2584837d4673665a77f2d578f4ce50e 2164 2155 2016-11-07T10:39:57Z Zuzanna 36 wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. '''Address:''' Sorbonnelaan 2 3584 CA Utrecht SRON Utrecht is located on the Uithof campus of the University of Utrecht. '''How to reach SRON Utrecht by public transport:''' Take the train to Utrecht central station: [http://www.ns.nl/en/journeyplanner/#/?vertrek=Schiphol%20Airport&vertrektype=treinstation&aankomst=Utrecht%20Centraal&aankomsttype=treinstation trains from Schiphol Airport (AMS)] Then take bus 28 (stop Botanische Tuinen) or bus 12 (stop Padualaan): [http://9292.nl/en/journeyadvice/station-utrecht-centraal/utrecht_sorbonnelaan-2 bus timetable] f22578b851dcf534897e623d1b221877ce50ec8e 2165 2164 2016-11-07T11:04:59Z Zuzanna 36 wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. ---- '''Address:''' Sorbonnelaan 2 3584 CA Utrecht SRON Utrecht is located on the Uithof campus of the University of Utrecht. ---- '''Coming to Utrecht by plane:''' If you intend to come by plane to the Netherlands/Utrecht, there are multiple airports in the vicinity: - Schiphol airport near Amsterdam serves almost all flight carriers (0.5h to Utrecht central station). - Eindhoven Airport, which serves Ryanair and a few other smaller airlines (1.5h to Utrecht central station). - Rotterdam Airport, for instance Transavia (1h to Utrecht central station). '''How to reach SRON Utrecht by public transport:''' Take the train to Utrecht central station: [http://www.ns.nl/en/journeyplanner/#/?vertrek=Schiphol%20Airport&vertrektype=treinstation&aankomst=Utrecht%20Centraal&aankomsttype=treinstation trains from Schiphol Airport (AMS)] Then take bus 28 (stop Botanische Tuinen) or bus 12 (stop Padualaan): [http://9292.nl/en/journeyadvice/station-utrecht-centraal/utrecht_sorbonnelaan-2 bus timetable] [http://9292.nl/en Public transport in the Netherlands] 7f6e48345da83fd1990268589c277660c18286d7 2166 2165 2016-11-07T11:07:28Z Zuzanna 36 wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. ---- '''Address:''' Sorbonnelaan 2 3584 CA Utrecht SRON Utrecht is located on the Uithof campus of the University of Utrecht. ---- '''Coming to Utrecht by plane:''' If you intend to come by plane to the Netherlands/Utrecht, there are multiple airports in the vicinity: - Schiphol Airport (AMS) near Amsterdam serves almost all flight carriers (0.5h to Utrecht central station). - Eindhoven Airport (EIN), which serves Ryanair and a few other smaller airlines (1.5h to Utrecht central station). - Rotterdam Airport (RTM), for instance Transavia (1.5h to Utrecht central station). '''How to reach SRON Utrecht by public transport:''' Take the train to Utrecht central station: [http://www.ns.nl/en/journeyplanner/#/?vertrek=Schiphol%20Airport&vertrektype=treinstation&aankomst=Utrecht%20Centraal&aankomsttype=treinstation eg. trains from Schiphol Airport] Then take bus 28 (stop Botanische Tuinen) or bus 12 (stop Padualaan): [http://9292.nl/en/journeyadvice/station-utrecht-centraal/utrecht_sorbonnelaan-2 bus timetable] [http://9292.nl/en Public transport in the Netherlands] 5c6d1d9bf97797d43d07d96848f58a5e59e5a992 2179 2166 2016-11-15T18:21:25Z Zuzanna 36 wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. ---- '''Address:''' Sorbonnelaan 2 3584 CA Utrecht SRON Utrecht is located on the Uithof campus of the University of Utrecht. ---- '''Coming to Utrecht by plane:''' If you intend to come by plane to the Netherlands/Utrecht, there are multiple airports in the vicinity: - Schiphol Airport (AMS) near Amsterdam serves almost all flight carriers (0.5h to Utrecht central station). - Eindhoven Airport (EIN), which serves Ryanair and a few other smaller airlines (1.5h to Utrecht central station). - Rotterdam Airport (RTM), for instance Transavia (1.5h to Utrecht central station). '''How to reach SRON Utrecht by public transport:''' Take the train to Utrecht central station: [http://www.ns.nl/en/journeyplanner/#/?vertrek=Schiphol%20Airport&vertrektype=treinstation&aankomst=Utrecht%20Centraal&aankomsttype=treinstation eg. trains from Schiphol Airport] Then take bus 28 (stop Botanische Tuinen) or bus 12 (stop Padualaan): [http://9292.nl/en/journeyadvice/station-utrecht-centraal/utrecht_sorbonnelaan-2 bus timetable] [http://9292.nl/en Public transport in the Netherlands] ---- '''Accommodation''' Hotel Park Plaza - close to the train station and bus stop 12, 28 [https://www.parkplaza.com/utrecht-hotel-nl-3531-bl/netutrec] NH Hotel Utrecht - close to the train station and bus stop 12, 28 [http://www.nh-hotels.com/booking/step1-rates?hotelId=NLUT.UTREC] NH Hotel Utrecht Centre - city centre and close to the bus stop 28 [http://www.nh-hotels.com/booking/step1-rates?hotelId=NLUT.CENUT] Hotel Malie - close to the bus stop 28 [http://www.maliehotel.nl/en] Hotel Oorsprongpark - close to the bus stop 28 [http://www.oorsprongpark.nl/en/] c30582fb7143c8be1a24d803318d186585f8151a 2181 2179 2016-11-15T18:41:32Z Zuzanna 36 wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. ---- '''Address:''' Sorbonnelaan 2 3584 CA Utrecht SRON Utrecht is located on the Uithof campus of the University of Utrecht. ---- '''Coming to Utrecht by plane:''' If you intend to come by plane to the Netherlands/Utrecht, there are multiple airports in the vicinity: - Schiphol Airport (AMS) near Amsterdam serves almost all flight carriers (0.5h to Utrecht central station). - Eindhoven Airport (EIN), which serves Ryanair and a few other smaller airlines (1.5h to Utrecht central station). - Rotterdam Airport (RTM), for instance Transavia (1.5h to Utrecht central station). '''How to reach SRON Utrecht by public transport:''' Take the train to Utrecht central station: [http://www.ns.nl/en/journeyplanner/#/?vertrek=Schiphol%20Airport&vertrektype=treinstation&aankomst=Utrecht%20Centraal&aankomsttype=treinstation eg. trains from Schiphol Airport] Then take bus 28 (stop Botanische Tuinen) or bus 12 (stop Padualaan): [http://9292.nl/en/journeyadvice/station-utrecht-centraal/utrecht_sorbonnelaan-2 bus timetable] [http://9292.nl/en Public transport in the Netherlands] ---- Tourist Information [http://www.visit-utrecht.com/ Visit Utrecht] ---- '''Accommodation''' Hotel Park Plaza - close to the train station Utrecht Centraal and bus stop 12, 28 [https://www.parkplaza.com/utrecht-hotel-nl-3531-bl/netutrec] NH Hotel Utrecht - close to the train station Utrecht Centraal and bus stop 12, 28 [http://www.nh-hotels.com/booking/step1-rates?hotelId=NLUT.UTREC] NH Hotel Utrecht Centre - city centre and close to the bus stop 28 [http://www.nh-hotels.com/booking/step1-rates?hotelId=NLUT.CENUT] Hotel Malie - close to the bus stop 28 [http://www.maliehotel.nl/en] Hotel Oorsprongpark - close to the bus stop 28 [http://www.oorsprongpark.nl/en/] ---- [[File:mapUtrecht.png|900px]] c4065db66b422f24572c50a4a44354f1f0c70e02 2184 2181 2016-11-15T18:44:40Z Zuzanna 36 wikitext text/x-wiki The workshop will take place in SRON, Netherlands Institute for Space Research in Utrecht in the Netherlands. ---- '''Address:''' Sorbonnelaan 2 3584 CA Utrecht SRON Utrecht is located on the Uithof campus of the University of Utrecht. ---- '''Coming to Utrecht by plane:''' If you intend to come by plane to the Netherlands/Utrecht, there are multiple airports in the vicinity: - Schiphol Airport (AMS) near Amsterdam serves almost all flight carriers (0.5h to Utrecht central station). - Eindhoven Airport (EIN), which serves Ryanair and a few other smaller airlines (1.5h to Utrecht central station). - Rotterdam Airport (RTM), for instance Transavia (1.5h to Utrecht central station). '''How to reach SRON Utrecht by public transport:''' Take the train to Utrecht central station: [http://www.ns.nl/en/journeyplanner/#/?vertrek=Schiphol%20Airport&vertrektype=treinstation&aankomst=Utrecht%20Centraal&aankomsttype=treinstation eg. trains from Schiphol Airport] Then take bus 28 (stop Botanische Tuinen) or bus 12 (stop Padualaan): [http://9292.nl/en/journeyadvice/station-utrecht-centraal/utrecht_sorbonnelaan-2 bus timetable] [http://9292.nl/en Public transport in the Netherlands] ---- Tourist Information [http://www.visit-utrecht.com/ Visit Utrecht] ---- '''Accommodation''' Hotel Park Plaza - close to the train station Utrecht Centraal and bus stop 12, 28 [https://www.parkplaza.com/utrecht-hotel-nl-3531-bl/netutrec] NH Hotel Utrecht - close to the train station Utrecht Centraal and bus stop 12, 28 [http://www.nh-hotels.com/booking/step1-rates?hotelId=NLUT.UTREC] NH Hotel Utrecht Centre - city centre and close to the bus stop 28 [http://www.nh-hotels.com/booking/step1-rates?hotelId=NLUT.CENUT] Hotel Malie - close to the bus stop 28 [http://www.maliehotel.nl/en] Hotel Oorsprongpark - close to the bus stop 28 [http://www.oorsprongpark.nl/en/] ---- [[File:mapUtrecht.png|900px]] [[File:bus12.png|400px]] [[File:bus28.png|400px]] b85dc92e96eade32b3830737df0bd1c7f4beb4df 0 271 2156 2149 2016-09-12T14:07:55Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2016.png|right|450px]] --> '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Participants]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> e8baca8c53b9d12c3a154976e556a8e85c486639 2157 2156 2016-09-12T14:09:34Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2016.png|right|450px]] --> '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations this time the workshop will be limited to 50 people only. Everyone interested in attending the meeting will have a chance to apply for an invitation, which then will be reviewed by the organizers. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> 89bd851c91aab86af2b52368afef8538e2c09dcb 2159 2157 2016-09-12T14:36:42Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2016.png|right|450px]] --> '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[[workshop2016:registration|Registration]] registration form] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> 00406d31290a1fb762dcde86fdc536d16e25564b 2160 2159 2016-09-12T14:37:07Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2016.png|right|450px]] --> '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> 5d52f47e0a8a2ee3970f7bd1ce7239b44b21986f 2161 2160 2016-09-12T14:37:21Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2016.png|right|450px]] --> '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> 68f76781f286a0760338e01479c051742041790f 2171 2161 2016-11-10T09:37:44Z Zuzanna 36 wikitext text/x-wiki == Welcome! == [[File:Poster2016.png|right|450px]] '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> 4fbfae95ea0275579f0693ba382e9150b64cac84 2173 2171 2016-11-10T09:47:05Z Zuzanna 36 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:poster2016.png|right|450px]] '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) <!--LOC: * Iain Steele * Andrzej Piascik * Helen Jermak * Rob Barnsley * Chris Copperwheat [[File:GaiaWorkshop2015.jpg|700px]] --> f6d0cb0c29703319722dee12c8b84d664ba63933 0 272 2158 2151 2016-09-12T14:24:58Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. === List of registered participants === (will be filled after 7.Nov) # c2dc793bedbb48527f86c7d5946549fbc0223555 2163 2158 2016-09-12T15:11:27Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs. === List of registered participants === (will be filled after 7.Nov) # 6656162631d0316c6a1c8701257d84d6e685113e 2167 2163 2016-11-09T21:19:42Z Zuzanna 36 /* List of registered participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs. === List of registered participants === # Giuseppe Altavilla # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Erika Pakstiene # Zsolt Paragi # Arne Rau # Krzysztof Rybicki # Iain Steele # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez 93e529573cc6613755f687514f5644c6a83ff53b 2168 2167 2016-11-09T21:22:56Z Zuzanna 36 wikitext text/x-wiki <!--<big>'''Registration is now open!'''</big>--> <big>'''Registration is now closed!'''</big> But if you are still desperate to come, drop us an email at gaia-alerts7@sron.nl <!--Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs.--> === List of registered participants === # Giuseppe Altavilla # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Erika Pakstiene # Zsolt Paragi # Arne Rau # Krzysztof Rybicki # Iain Steele # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez a2d3e250e9740c7aa45387bc696e2e7cc2b0a077 2169 2168 2016-11-09T21:43:40Z Zuzanna 36 /* List of registered participants */ wikitext text/x-wiki <!--<big>'''Registration is now open!'''</big>--> <big>'''Registration is now closed!'''</big> But if you are still desperate to come, drop us an email at gaia-alerts7@sron.nl <!--Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs.--> === List of registered participants === # Giuseppe Altavilla # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Erika Pakstiene # Zsolt Paragi # Arne Rau # Krzysztof Rybicki # Iain Steele # Beatriz Villarroel # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez caa0bfd6a41ea9adf7c80822194e694d67917aee 2175 2169 2016-11-12T14:35:44Z Zuzanna 36 /* List of registered participants */ wikitext text/x-wiki <!--<big>'''Registration is now open!'''</big>--> <big>'''Registration is now closed!'''</big> But if you are still desperate to come, drop us an email at gaia-alerts7@sron.nl <!--Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs.--> === List of registered participants === # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Erika Pakstiene # Zsolt Paragi # Isabella Pagano # Arne Rau # Krzysztof Rybicki # Iain Steele # Beatriz Villarroel # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez 0b62ec5296050c15c0d7242f2befb06192c25831 2176 2175 2016-11-12T14:36:09Z Zuzanna 36 /* List of registered participants */ wikitext text/x-wiki <!--<big>'''Registration is now open!'''</big>--> <big>'''Registration is now closed!'''</big> But if you are still desperate to come, drop us an email at gaia-alerts7@sron.nl <!--Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs.--> === List of registered participants === # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Isabella Pagano # Erika Pakstiene # Zsolt Paragi # Arne Rau # Krzysztof Rybicki # Iain Steele # Beatriz Villarroel # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez e65506d6fc0bff963f533597515bc0fdf647591e 2177 2176 2016-11-14T13:21:51Z Zuzanna 36 wikitext text/x-wiki <!--<big>'''Registration is now open!'''</big>--> <big>'''Registration is now closed!'''</big> But if you are still desperate to come, drop us an email at gaia-alerts7@sron.nl <!--Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs.--> === List of registered participants === # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Isabella Pagano # Erika Pakstiene # Zsolt Paragi # Arne Rau # Krzysztof Rybicki # Iain Steele # Giovanna Maria Stirpe # Beatriz Villarroel # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez 8e1a77f5f10e7d5dc98d897cf654b22efc440d62 2190 2177 2016-11-25T13:36:59Z Zuzanna 36 /* List of registered participants */ wikitext text/x-wiki <!--<big>'''Registration is now open!'''</big>--> <big>'''Registration is now closed!'''</big> But if you are still desperate to come, drop us an email at gaia-alerts7@sron.nl <!--Registration closes on '''1.November 2016'''. In case of any questions, please email gaia-alerts7@sron.nl Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the registration form below and provide your case why do you want to attend the workshop. <big> [https://goo.gl/forms/xWY98Negxx0eiz8a2 Registration form] </big> We will confirm your registration by e-mail by Nov.7. ===Support === Thanks to the OPTICON grant, there will be a limited support available for some attendees (travel costs only). Please send your support request in a separate email (after registering) to gaia-alerts7@sron.nl with justification of your attendance and an estimate on the costs.--> === List of registered participants === # Volkan Bakis # Sergi Blanco-Cuaresma # Giacomo Cannizzaro # James Chibueze # Goran Damljanovic # Jos de Bruijne # Michel Dennefeld # Orhan Erece # Steve Fossey # Gerry Gilmore # Andreja Gomboc # Aleksandra Hamanowicz # Simon Hodgkin # Peter Jonker # Habib Khosroshahi # Zuzanna Kostrzewa-Rutkowska # Giuseppe Leto # Fraser Lewis # Alireza Molaeinezhad # Meredith Morrell # Francesca Onori # Isabella Pagano # Erika Pakstiene # Zsolt Paragi # Arne Rau # Krzysztof Rybicki # Giovanna Maria Stirpe # Beatriz Villarroel # Thomas Wevers # Lukasz Wyrzykowski # Ricardo Zanmar Sanchez 83bfc1ed4285ad3022b993bd62e5642623e40dcb 6 276 2170 2016-11-10T09:37:02Z Zuzanna 36 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2172 2170 2016-11-10T09:45:59Z Zuzanna 36 Zuzanna uploaded a new version of [[File:Poster2016.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2174 2172 2016-11-10T09:48:22Z Zuzanna 36 Zuzanna uploaded a new version of [[File:Poster2016.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 214 2178 2144 2016-11-14T21:42:54Z Gsawgwikiadmin 1 wikitext text/x-wiki Tentative list of Working Groups with people interested to be part of them. Please email LW if you would like to be added to any of the groups. Soon the pages below will become the workplace for each of the WGs. Email LW if you want to obtain the credentials to edit the wiki pages. The numbers indicate the order of joining the group. Volunteers for leading the group are marked in bold. [O] - happy to observe [S] - student Link to INT spectroscopy proposal I/2014A/4 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_int.pdf PDF] Link to WHT spectroscopy proposal W/2014A/31 (submitted 15/9/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/File:Fuga_wht.pdf PDF] Link to NTT spectroscopy proposal ID: 093.D-0856 (submitted 1/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/d/da/Fuga_ntt.pdf PDF] Link to PATT Liverpool Telescope spectroscopy proposal ID: PL14A15 (submitted 4/10/2013): [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/3/36/Fugalt.pdf PDF] Link to JMU Liverpool Telescope spectroscopy proposal ID: #10 (submitted 4/10/2013) : [http://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/images/e/ea/14A-GAIA-JMU.pdf PDF] === GSAWG1: Supernovae (Core collapse, 1a) === #'''Nic Walton [O]''' #Simon Clark #Eran Ofek #Stephen Smartt #Mark Sullivan [O] #Sjoert van Velzen [O] #Patricia Whitelock #Andrzej Pigulski #Massimo Turatto #Lukasz Wyrzykowski [O] #Michel Dennefeld [O] #Morgan Fraser [O] #Lina Tomasella #Heather Campbell [O] #Stefano Benetti #Andrea Pastorello #Nadia Blagorodnova [O][S] #Christian Knigge #Paolo Mazzali #David Bersier #Rob Barnsley #Philip James #Sergey Koposov #Valerio A. R. M. Ribeiro #Ian Skillen #Giuseppe Altavilla #Mickael Rigault #Oliver Vince #Goran Damljanovic #Philipp Podsiadlowski #Seppo Mattila #Erkki Kankare #Cosimo Inserra #Rubina Kotak #Lovro Palaversa #Bruce Bassett # Fraser Lewis === GSAWG2: CVs and XRBs === This group has already established their own mailing list. Please contact the chair, Elme, if you want to join it. #'''Elme Breedt [O]''' #Simon Clark #Peter Jonker [O] #Zbigniew Kolaczkowski #Ulrich Kolb #Richard Busuttil #Boris Gaensicke [O] #Retha Pretorius #Andrzej Pigulski #Stuart P Littlefair [O] #Chris Copperwheat #Peter Wheatley [O] #Stephen Potter #Michel Dennefeld [O] #Danny Steeghs [O] #Matthew Schurch [O] #Thomas Wevers [S][O] #Rob Fender #Christian Knigge #Vik Dhillon #Phil Charles #Andrew Mason #Marian Doru Suran #Dumitru Pricopi #Alexandru Dumitrescu #Valerio A. R. M. Ribeiro #Ian Skillen #Lovro Palaversa #Patrick Woudt #Rene Hudec #Axel Schwope #Fraser Lewis === GSAWG3: Microlensing === #'''Lukasz Wyrzykowski''' #Eran Ofek #Rachel Street #Martin Dominik #Arnaud Cassan #Yannis Tsapras #Fraser Lewis === [http://wiki.astro.ljmu.ac.uk/YoungTransients/ GSAWG4: Young Stars] === ''NOTE: Wiki pages of this WG are password protected. If you want to join this group please email Chris Davis at Liverpool John Moores University'' #'''Chris Davis [O]''' #Aleks Scholz [O] #Zbigniew Kolaczkowski #Michael Smith #Dirk Froebrich [O] #Philip Lucas #Tigran Magakian #Suzie Ramsay #Steve Longmore #Carlos Contreras #Tim Naylor [O] #Darryl Sergison #Laszlo Szabados #Cecilia Farina [O] #Joao Alves #Tim Gledhill #Timo Prusti #Tom Ray #Tae-Soo Pyo #Nick Wright #Hauyu Baobab Liu #Jochen Eisloeffel #David Ardila #Fraser Lewis === GSAWG5: AGNs and TDEs === #'''Sjoert van Velzen''' [O] #Paul O'Brien #Norbert Schartel #Peter Jonker [O] #Helene Sol #Stefanie Komossa #Stephen Smartt #Mark Sullivan [O] #Stephen Potter #Elme Breedt [O] #Michel Dennefeld [O] #Andreja Gomboc #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Ashish Mahabal #Nic Walton [O] #Werner Zeilinger #Carole Mundell #David Bersier #Shiho Kobayashi #Stefano Benetti #Sergey Koposov #Oliver Vince #Goran Damljanovic #Francois Taris #Alexandre Humberto Andrei #Poshak Gandhi #Lovro Palaversa #Peter Maksym[O] #Sheila McBreen #David Lynn #Derek O'Callaghan === GSAWG6: GRBs === #'''Andreja Gomboc''' #Paul O'Brien #Stephen Smartt #Mark Sullivan [O] #David Alexander Kann #Matthew Schurch [O] #Jure Japelj #Neil Gehrels #Carole Mundell #Paolo Mazzali #David Bersier #Shiho Kobayashi #Stefano Benetti #Susanna Vergani #Istvan Horvath #Rene Hudec === GSAWG7: Be stars, R CrB stars, other rare events === #Simon Clark #Patrick Tisserand #Zbigniew Kolaczkowski #Boris Gaensicke #Patricia Whitelock #Andrzej Pigulski #Peter Wheatley [O] #Laurent Eyer #Matthew Schurch #Laszlo Szabados #Andrea Pastorello #Rob Barnsley #Pavel Koubsky #Yves Frémat #Andrew Mason #Lovro Palaversa #Retha Pretorius #Rene Hudec #Fraser Lewis === GSAWG8: Gaia Alerts Processing and Infrastructure === #'''Simon Hodgkin''' [O] #Dafydd Wyn Evans #Francesca De Angeli #Giorga Busso #Marco Riello #Anthony Brown (DPAC chair) #Nadia Blagorodnova [O][S] #Patrick Burgess #Laurent Eyer #Timo Prusti (ESA: Gaia Project Scientist) #Sergey Koposov #Nic Walton (DPAC CU5/CU9 / GST) #Lukasz Wyrzykowski === GSAWG9: Spectroscopic Follow-Up === #'''Simon Hodgkin [O]''' #Lina Tomasella #Stefanie Komossa #Danny Steeghs #Andreja Gomboc #Cecilia Farina [O] #Morgan Fraser [O] #Nadia Blagorodnova [O][S] #Nic Walton [O] #Chris Davis #David Bersier #Werner Zeilinger #Philippe Bendjoya #Giuseppe Altavilla #Mickael Rigault #Jean-Pierre Rivet #Michel Dennefeld [O] #Thomas Wevers [O] #Lovro Palaversa[O][S] #Andrzej Piascik #Heather Campbell [O] #George Seabroke #Olivier Marchal #Paola di Matteo #Axel Schwope #Fraser Lewis === GSAWG10: Photometric Follow-Up === Google Group emailing list established (gsawg10-photometric-follow-up). Email LW if you did not receive the invitation yet. The list below might not be complete. #'''Lukasz Wyrzykowski''' #Andreja Gomboc #Liam K Hardy [O][S] #Ulrich Kolb [O] #Peter Wheatley [O] #Cecilia Farina [O] #Ashish Mahabal #Gabor Marschalko [O] #David Bersier #Andrzej Pigulski #Zbyszek Kołaczkowski #Grzegorz Kopacki #Przemek Brus #Dawid Moździerski #Gabriela Michalska #Pavel Koubsky #Philip James #Sergey Koposov #Philippe Bendjoya #Giuseppe Leto #Giuseppe Altavilla #Oliver Vince #Goran Damljanovic #Jean-Pierre Rivet #Jure Japelj #Johanna Jarvis #Lovro Palaversa[O][S] #Heather Campbell [O] #Josep Manel Carrasco #Eduard Masana #Rene Hudec #Fraser Lewis #Richard.Busuttil #Simon Hodgkin #Erika Pakstiene 59e5e6989b4878fd6249e7dd7b97ec7ff7058109 6 277 2180 2016-11-15T18:23:01Z Zuzanna 36 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 278 2182 2016-11-15T18:41:51Z Zuzanna 36 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 279 2183 2016-11-15T18:42:04Z Zuzanna 36 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 200 2191 1636 2016-11-29T16:33:56Z Lukasz 2 wikitext text/x-wiki The main address of the server at the moment is: http://gsaweb.ast.cam.ac.uk/followup == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your sextractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 2f044f89bccb79f1cdba72633775966bfe8cdffb 6 280 2198 2016-12-07T11:05:33Z Zuzanna 36 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 274 2202 2201 2016-12-08T09:16:28Z Gsawgwikiadmin 1 wikitext text/x-wiki '''AGENDA''' <big>[[Media:abstractbook2016.pdf|Abstract book [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution |0:25 |---- |10:10 |Peter Jonker |Nuclear transients |0:25 |---- |10:35 |'''workshop photo''' | |0:10 |---- |10:45 |'''coffee break''' | |0:30 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope |0:20 |---- |10:50 |'''coffee break''' | |0:30 |---- |11:20 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds |0:60 |---- |12:20 | |Closing remarks |0:15 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 591251abd2fa4793036b58101a2a6ccf8f3796c4 2207 2202 2016-12-12T13:02:07Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' <big>[[Media:abstractbook2016.pdf|Abstract book [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day1-1-jos-debruijne.pdf pdf] |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day1-2-simon_hodgkin.pdf pdf] |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-3-lukasz-wyrzykowski.pdf pdf] |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day1-4-isabella-pagano.pdf pdf] |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day1-5-erika-pakstiene.pdf pdf] |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day1-6-arne-rau.pdf pdf] |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day1-7-beatriz_villarroel.pdf pdf] |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-am-1-gerry-gilmore.pdf pdf] |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-am-2-zsolt-paragi.pdf pdf] |0:25 |---- |10:10 |Peter Jonker |Nuclear transients [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-am-3-peter-jonker.pdf pdf] |0:25 |---- |10:35 |'''workshop photo''' | |0:10 |---- |10:45 |'''coffee break''' | |0:30 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-am-4-francesca-onori.pdf pdf] |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-am-5-aleksandra-hamanowicz.pdf pdf] |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-am-6-zuzanna-kostrzewa-rutkowska.pdf pdf] |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-1-thomas-wevers.pdf pdf] |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-2-krzysztof-rybicki.pdf pdf] |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-3-lukasz-wyrzykowski.pdf pdf] |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-4-habib-khosroshahi.pdf pdf] |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-5-fraser-lewis.pdf pdf] |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-6-meredith-morrell.pdf pdf] |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-7-michel-dennefeld.pdf pdf] |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-8-ricardo-zanmar-sanchez.pdf pdf] |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day2-pm-9-lukasz-wyrzykowski-opticon.pdf pdf] |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day3-1-giovanna-stirpe.pdf pdf] |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day3-2-goran-damljanovic.pdf pdf] |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day3-3-volkan-bakis.pdf pdf] |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day3-4-orhan-erece.pdf pdf] |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day3-5-andreja-gomboc.pdf pdf] |0:20 |---- |10:50 |'''coffee break''' | |0:30 |---- |11:20 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds [http://www.astrouw.edu.pl/wyrzykow/GAIA/GSAW2016/slides/day3-6-lukasz-wyrzykowski.pdf pdf] |0:60 |---- |12:20 | |Closing remarks |0:15 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 9a275559f14a7a7dd9f650b21c53db06d478276d 2208 2207 2016-12-12T13:26:52Z Zuzanna 36 wikitext text/x-wiki '''AGENDA''' <big>[[Media:abstractbook2016.pdf|Abstract book [pdf]]]</big> {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 7 December 2016''' |---- |---- |12:00 |'''lunch & registration''' | |2:00 |---- |14:00 | |Welcome |0:10 |---- |14:10 |Jos de Bruijne |Gaia status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-1-jos-debruijne.pdf pdf] |0:30 |---- |14:40 |Simon Hodgkin |Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-2-simon_hodgkin.pdf pdf] |0:45 |---- |15:25 |Lukasz Wyrzykowski |Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-3-lukasz-wyrzykowski.pdf pdf] |0:30 |---- |15:55 |'''coffee break''' | |0:40 |---- |16:35 |Isabella Pagano |The PLATO mission: synergies with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-4-isabella-pagano.pdf pdf] |0:20 |---- |16:55 |Erika Pakstiene |Spectroscopic and Photometric observations at Moletai AO for the ESA PLATO space mission [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-5-erika-pakstiene.pdf pdf] |0:20 |---- |17:15 |Arne Rau |SRG/eROSITA - Gaia synergies for transients and variables [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-6-arne-rau.pdf pdf] |0:25 |---- |17:40 |Beatriz Villarroel |The VASCO mission: Searches for Vanishing Stars with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day1-7-beatriz_villarroel.pdf pdf] |0:25 |---- |18:05 |'''end of day 1''' | | |---- |colspan="4"|'''Thursday, 8 December 2016''' |---- |09:30 |Gerry Gilmore |OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-am-1-gerry-gilmore.pdf pdf] |0:15 |---- |09:45 |Zsolt Paragi |Tidal Disruption Events followed-up with milli-arcsec resolution [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-am-2-zsolt-paragi.pdf pdf] |0:25 |---- |10:10 |Peter Jonker |Nuclear transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-am-3-peter-jonker.pdf pdf] |0:25 |---- |10:35 |'''workshop photo''' | |0:10 |---- |10:45 |'''coffee break''' | |0:30 |---- |11:15 |Francesca Onori |Spectroscopic follow-up of iPTF16fnl: a uniquely nearby tidal disruption event [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-am-4-francesca-onori.pdf pdf] |0:20 |---- |11:35 |Aleksandra Hamanowicz |Nuclear transients from Gaia: the classification and follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-am-5-aleksandra-hamanowicz.pdf pdf] |0:20 |---- |11:55 |Zuzanna Kostrzewa-Rutkowska |Gaia nuclears - how to [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-am-6-zuzanna-kostrzewa-rutkowska.pdf pdf] |0:20 |---- |12:15 |'''lunch''' | |1:35 |---- |13:50 |Thomas Wevers |Fast transients with Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-1-thomas-wevers.pdf pdf] |0:25 |---- |14:15 |Krzysztof Rybicki |Simulating Gaia astrometry of microlensing events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-2-krzysztof-rybicki.pdf pdf] |0:25 |---- |14:40 |Lukasz Wyrzykowski |Gaia16aye - spectacular binary microlensing event [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-3-lukasz-wyrzykowski.pdf pdf] |0:25 |---- |15:05 |Habib Khosroshahi |Iranian National Observatory; project update [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-4-habib-khosroshahi.pdf pdf] |0:20 |---- |15:25 |'''coffee break''' | |0:40 |---- |16:05 |Fraser Lewis |Monitoring Gaia Alerts Targets with the Faulkes Telescope Project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-5-fraser-lewis.pdf pdf] |0:15 |---- |16:20 |Meredith Morrell |PIRATE observatory of the Open University [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-6-meredith-morrell.pdf pdf] |0:15 |---- |16:35 |Michel Dennefeld |OHP contribution to Gaia Alerts follow-up [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-7-michel-dennefeld.pdf pdf] |0:20 |---- |16:55 |Ricardo Zanmar Sanchez |The robotic telescope APT2 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-8-ricardo-zanmar-sanchez.pdf pdf] |0:15 |---- |17:10 |Lukasz Wyrzykowski |OPTICON follow-up network 2012-2020, plans for future, feedback, discussions [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day2-pm-9-lukasz-wyrzykowski-opticon.pdf pdf] |0:40 |---- |17:50 |'''end of day 2''' | | |---- |19:00 |'''WORKSHOP DINNER''' | | |---- |---- |colspan="4"|'''Friday, 9 December 2016''' |---- |09:30 |Giovanna Maria Stirpe |The 1.52m Loiano Telescope and the Gaia Alerts challenge [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day3-1-giovanna-stirpe.pdf pdf] |0:15 |---- |09:45 |Goran Damljanovic |Observations of Gaia Alerts by using Serbian-Bulgarian mini-network telescopes during 2016 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day3-2-goran-damljanovic.pdf pdf] |0:15 |---- |10:00 |Volkan Bakis |Recent Studies and Available Facilities of the Akdeniz University Space Sciences Group [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day3-3-volkan-bakis.pdf pdf] |0:15 |---- |10:15 |Orhan Erece |Gaia Sources Observations with TUG Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day3-4-orhan-erece.pdf pdf] |0:15 |---- |10:30 |Andreja Gomboc |Gaia Alert Spectroscopy with SPRAT at the Liverpool Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day3-5-andreja-gomboc.pdf pdf] |0:20 |---- |10:50 |'''coffee break''' | |0:30 |---- |11:20 |Lukasz Wyrzykowski + Krzysztof Rybicki |Workshop - hands-on: Calib Server, data reds [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2016/slides/day3-6-lukasz-wyrzykowski.pdf pdf] |0:60 |---- |12:20 | |Closing remarks |0:15 |---- |12:35 |'''lunch''' | |1:25 |---- |14:00 |'''end of the meeting''' | | |} '''NOTE: agenda might still change slightly''' 30aef0a2c4b84bc1ffff0c8a3a2bfe178491a95a 0 271 2203 2173 2016-12-12T10:49:01Z Zuzanna 36 wikitext text/x-wiki == Welcome! == [[File:poster2016.png|right|450px]] '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) [[File:GaiaWorkshop2016.jpg|700px]] 71f77d8bc368675c2954cc1c463086d98f342f72 2205 2203 2016-12-12T10:51:47Z Zuzanna 36 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:poster2016.png|right|450px]] '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) 13d9611fd47ca774753844b8f74d0ce7265ab9d9 2206 2205 2016-12-12T10:52:18Z Zuzanna 36 wikitext text/x-wiki == Welcome! == [[File:poster2016.png|right|450px]] '''The seventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2016:logistics | Utrecht, Netherlands, 7-9 December 2016]].''' The topics this year include: * present and discuss scientific results from the Gaia Alerts so far * discuss further scientific drivers and dedicated topics from Gaia Alerts (TDEs, microlensing events, SNe, CVs) * discuss synergies between major large-scale transient surveys in order to maximise the scientific outcome of the Gaia Alerts * present the status and the organisation of the H2020 OPTICON follow-up network * receive feedback from the users to Gaia Alerts * discuss and recognise future steps in improving the follow-up programmes Due to space limitations of the workshop venue, we have to limit the number of attendees to 50. We hope that everyone will be accepted, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2016:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2016:rationale|Rationale]] * [[workshop2016:agenda|Agenda]] * [[workshop2016:registration|Registration]] * [[workshop2016:logistics|Logistic information]] <!--* [[workshop2016:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Peter Jonker (SRON) * Morgan Fraser (Dublin) * Simon Hodgkin (Cambridge) * Zuzanna Kostrzewa-Rutkowska (SRON) * Lukasz Wyrzykowski (Warsaw) [[File:GaiaWorkshop2016.jpg|700px]] d8e67424069208cf15416db34a91d7c853f319e8 6 281 2204 2016-12-12T10:49:56Z Zuzanna 36 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 200 2209 2191 2017-01-19T14:02:43Z Lukasz 2 wikitext text/x-wiki The main address of the server is: http://gsaweb.ast.cam.ac.uk/followup == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. Updated December 2016 by LW. == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org 06d6b1a2df308a90f17773ad402100e02b2cc50e 0 1 2210 2146 2017-08-11T21:20:28Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw, 29.Nov-1.Dec 2017]]</Big>''' </center> ---- <center> [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 883507580706701f5a0172d07e14edc24f3aa10d 8 3 2211 2152 2017-08-11T21:23:04Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2017 **workshop2017:main|Main Workshop Page **workshop2017:rationale|Rationale **workshop2017:agenda|Program **workshop2017:registration|Participants and Registration **workshop2017:logistics|Logistics *workshop 2016 **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 5d594f9242bbeb7aed254a9a96e6869cb41c1c7a 0 282 2212 2017-08-11T21:30:13Z Gsawgwikiadmin 1 Created page with "== Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eight OPTICON Gaia Science Alerts workshop will be held in Workshop2017:logistics | Warsaw, Poland, 29. N..." wikitext text/x-wiki == Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eight OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 29. Nov - 1.Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- <!--* [[workshop2017:rationale|Rationale]]--> * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] <!--* [[workshop2017:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) 609ea72343123ac7a175aae5ca7c4e495a6dace4 2213 2212 2017-08-11T21:31:19Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 29. Nov - 1.Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- <!--* [[workshop2017:rationale|Rationale]]--> * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] <!--* [[workshop2017:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) a9a6582fe0a10acd34d78dba2f7d684f3a772656 2223 2213 2017-09-29T06:18:41Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 9 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- <!--* [[workshop2017:rationale|Rationale]]--> * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] <!--* [[workshop2017:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) f6e97c190482cb95ad358f4036ba9f2aa09aa463 2224 2223 2017-09-29T06:19:05Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 9 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- <!--* [[workshop2017:rationale|Rationale]]--> * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] <!--* [[workshop2017:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) beb10b141f489ac042f6bbdcd7976395f6444dd8 2227 2224 2017-10-10T05:39:23Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 8 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- <!--* [[workshop2017:rationale|Rationale]]--> * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] <!--* [[workshop2017:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) 2abdb426f794cc75901171de5a4da27f49af6cf0 2228 2227 2017-10-10T05:39:36Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!-- [[File:poster2017.png|right|450px]] --> '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 8 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2017:rationale|Rationale]] * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] <!--* [[workshop2017:poster|Workshop's poster for download]]--> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) 739aa47902dff156480c39785912c19a64d02e90 2229 2228 2017-10-10T10:19:57Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2017.png|right|450px]] '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 8 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2017:rationale|Rationale]] * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] * [[workshop2017:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) fe130e286201c1db34da9ca9aab73326201a0728 2231 2229 2017-10-10T10:22:08Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2017.png|right|450px|poster2017]] '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 8 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2017:rationale|Rationale]] * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] * [[workshop2017:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) 23774c313f1c78def1f513366a1b5c2886a275fe 2237 2231 2017-10-10T12:06:25Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:poster2017-small.png|right|450px|poster2017]] '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 8 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2017:rationale|Rationale]] * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] * [[workshop2017:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) 7fee4d99d36b1e5979e5be72f86d2c9315751ede 2239 2237 2017-10-10T12:08:09Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2017-small.png|right|450px|poster2017]] '''The eighth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2017:logistics | Warsaw, Poland, 6 - 8 Dec. 2017]].''' The scope of the workshop this year will be slightly different than in the past. The main emphasis will be put on the organization of the follow-up observations, data reductions, calibrations, etc. There will be hands-on session and ample of time for brain-storming discussions to put the follow-up group to a new level. Therefore we strongly encourage all people involved in the follow-up of Gaia alerts to attend the meeting. Also we invite new observers and scientists interested in the involvement in the OPTICON follow-up network and scientific exploitation of the Gaia alerts. Due to space limitations of the workshop venue, we have to limit the number of attendees to 40. We hope that everyone interested will fit within this number, but in case of larger interest, we will select the attendees among the registrants to assure a broad and equal representation of topics. Please fill the [[workshop2017:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2017:rationale|Rationale]] * [[workshop2017:agenda|Agenda]] * [[workshop2017:registration|Registration]] * [[workshop2017:logistics|Logistic information]] * [[workshop2017:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Kris Rybicki (Warsaw) 0a260fe89f419463e9da872afccde91660f0ca83 0 283 2214 2017-09-23T05:32:16Z Gsawgwikiadmin 1 Created page with "The workshop will start on lunch-time on Wednesday, 29.Nov and finish by lunch time on Friday, 1.Dec." wikitext text/x-wiki The workshop will start on lunch-time on Wednesday, 29.Nov and finish by lunch time on Friday, 1.Dec. f174d102786b24642ff80d6187740b6e7a7ce69a 2246 2214 2017-10-19T21:17:45Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will start on lunch-time on Wednesday, 6.Dec and finish by lunch time on Friday, 8.Dec. 18a684310d463b942536f831f72b097ace460916 0 284 2215 2017-09-23T05:41:19Z Gsawgwikiadmin 1 Created page with "== Travel == == Venue == Astronomical Observatory of the University of Warsaw (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronou..." wikitext text/x-wiki == Travel == == Venue == Astronomical Observatory of the University of Warsaw (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronounce.com/polish/obserwatorium-astronomiczne/ listen]) [https://goo.gl/maps/vDe55iV68hR2 Google map] 09e1f5f16ba0560f285ae662c75455d4ef5d83fb 2216 2215 2017-09-23T05:45:57Z Gsawgwikiadmin 1 wikitext text/x-wiki = Travel Info = == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop Venue = '''Astronomical Observatory of the University of Warsaw''' (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronounce.com/polish/obserwatorium-astronomiczne/ listen]) Address: Aleje Ujazdowskie 4 00-478 Warszawa [https://goo.gl/maps/vDe55iV68hR2 Google map] For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Chopin Airport: [https://jakdojade.pl/warszawa/trasa/z--Warsaw-Chopin-Airport--do--Aleje-Ujazdowskie-4?fn=Warsaw%20Chopin%20Airport&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.17135:20.97239&ft=LOCATION_TYPE_POI&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] 107b7bcab81653012513fcd4046d17f7aa3c2252 2217 2216 2017-09-23T05:52:15Z Gsawgwikiadmin 1 wikitext text/x-wiki = Travel Info = == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop Venue = '''Astronomical Observatory of the University of Warsaw''' (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronounce.com/polish/obserwatorium-astronomiczne/ listen]) Address: Aleje Ujazdowskie 4 00-478 Warszawa [https://goo.gl/maps/vDe55iV68hR2 Google map] For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Chopin Airport: [https://jakdojade.pl/warszawa/trasa/z--Warsaw-Chopin-Airport--do--Aleje-Ujazdowskie-4?fn=Warsaw%20Chopin%20Airport&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.17135:20.97239&ft=LOCATION_TYPE_POI&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] The nearest bus stop to the Observatory is called ''Plac na Rozdrozu'' ([https://www.howtopronounce.com/polish/plac-na-rozdrozu/ pronunciation]). From Chopin Airport there is a direct bus no 188, reaching Plac na Rozdrozu in 40 mins. From there it is a 5 minute work South to the Observatory. From Modlin Airport the best option is to use [https://www.modlinbus.com/ Modlin Bus] to reach Warsaw City Centre. From there you can either use trams (4, 18, 35) to Plac Unii Lubelskiej [https://jakdojade.pl/warszawa/trasa/z--CENTRUM--do--Aleje-Ujazdowskie-4?fn=CENTRUM&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.23124:21.01015&fsn=CENTRUM&ft=LOCATION_TYPE_STOP&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] or Metro M1 line, one stop to Politechnika, and then walk for about 10 mins. b689ab8a2c7209eba9fae85b998ccb1809b55a06 2218 2217 2017-09-23T05:59:10Z Gsawgwikiadmin 1 wikitext text/x-wiki = Travel Info = == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop Venue = '''Astronomical Observatory of the University of Warsaw''' (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronounce.com/polish/obserwatorium-astronomiczne/ listen]) Address: Aleje Ujazdowskie 4 00-478 Warszawa [https://goo.gl/maps/vDe55iV68hR2 Google map] The Observatory is located together with the Botanic Garden (the same entrance from the street). For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Chopin Airport: [https://jakdojade.pl/warszawa/trasa/z--Warsaw-Chopin-Airport--do--Aleje-Ujazdowskie-4?fn=Warsaw%20Chopin%20Airport&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.17135:20.97239&ft=LOCATION_TYPE_POI&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] The nearest bus stop to the Observatory is called ''Plac na Rozdrozu'' ([https://www.howtopronounce.com/polish/plac-na-rozdrozu/ pronunciation]). From Chopin Airport there is a direct bus no 188, reaching Plac na Rozdrozu in 40 mins. From there it is a 5 minute work South to the Observatory. From Modlin Airport the best option is to use [https://www.modlinbus.com/ Modlin Bus] to reach Warsaw City Centre. From there you can either use trams (4, 18, 35) to Plac Unii Lubelskiej [https://jakdojade.pl/warszawa/trasa/z--CENTRUM--do--Aleje-Ujazdowskie-4?fn=CENTRUM&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.23124:21.01015&fsn=CENTRUM&ft=LOCATION_TYPE_STOP&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] or Metro M1 line, one stop to Politechnika, and then walk for about 10 mins. = Accommodation = Here is the list of hotels in the city centre and closer to the Observatory: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] the nearest to the Observatory * [http://www.lazienkowski.pl/ Łazienkowski] An alternative is AirBnB, where you can find a small flat for less than 50 euro per night [https://www.airbnb.com/s/Warsaw--Poland/homes?refinements%5B%5D=for_you&allow_override%5B%5D=&children=0&infants=0&adults=2&guests=2&room_types%5B%5D=Entire%20home%2Fapt&checkin=2017-11-28&checkout=2017-12-01&ib=true&ne_lat=52.22098485853037&ne_lng=21.032928295019815&sw_lat=52.20984283248001&sw_lng=21.0177791785037&zoom=15&search_by_map=true&s_tag=cnAYtZa9] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 5af8bf2c6540a841915204f9f5ced8194e82f607 2219 2218 2017-09-23T06:00:52Z Gsawgwikiadmin 1 /* Workshop Venue */ wikitext text/x-wiki = Travel Info = == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Amsterdam, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop Venue = '''Astronomical Observatory of the University of Warsaw''' (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronounce.com/polish/obserwatorium-astronomiczne/ listen]) Address: Aleje Ujazdowskie 4 00-478 Warszawa [https://goo.gl/maps/vDe55iV68hR2 Google map] The Observatory is located together with the Botanic Garden (the same entrance from the street). For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Chopin Airport: [https://jakdojade.pl/warszawa/trasa/z--Warsaw-Chopin-Airport--do--Aleje-Ujazdowskie-4?fn=Warsaw%20Chopin%20Airport&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.17135:20.97239&ft=LOCATION_TYPE_POI&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] The nearest bus stop to the Observatory is called ''Plac na Rozdrozu'' ([https://www.howtopronounce.com/polish/plac-na-rozdrozu/ pronunciation]). From Chopin Airport there is a direct bus no 188, reaching Plac na Rozdrozu in 40 mins. From there it is a 5 minute walk South to the Observatory (will be located on the left). From Modlin Airport the best option is to use [https://www.modlinbus.com/ Modlin Bus] to reach Warsaw City Centre. From there you can either use trams (4, 18, 35) to Plac Unii Lubelskiej [https://jakdojade.pl/warszawa/trasa/z--CENTRUM--do--Aleje-Ujazdowskie-4?fn=CENTRUM&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.23124:21.01015&fsn=CENTRUM&ft=LOCATION_TYPE_STOP&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] or Metro M1 line, one stop to Politechnika, and then walk for about 10 mins. = Accommodation = Here is the list of hotels in the city centre and closer to the Observatory: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] the nearest to the Observatory * [http://www.lazienkowski.pl/ Łazienkowski] An alternative is AirBnB, where you can find a small flat for less than 50 euro per night [https://www.airbnb.com/s/Warsaw--Poland/homes?refinements%5B%5D=for_you&allow_override%5B%5D=&children=0&infants=0&adults=2&guests=2&room_types%5B%5D=Entire%20home%2Fapt&checkin=2017-11-28&checkout=2017-12-01&ib=true&ne_lat=52.22098485853037&ne_lng=21.032928295019815&sw_lat=52.20984283248001&sw_lng=21.0177791785037&zoom=15&search_by_map=true&s_tag=cnAYtZa9] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 851f311244644191b65c745d593ac654ca55e709 2222 2219 2017-09-26T12:59:09Z Zuzanna 36 /* By Train */ wikitext text/x-wiki = Travel Info = == By Air == Warsaw has two airports operating international flights: * [http://www.lotnisko-chopina.pl/en/passenger?cl=en&set_language=en Chopin]: main airport, major airlines, located within the city * [http://en.modlinairport.pl/ Modlin]: cheap airline airport, only RyanAir flights from all over the Europe, located 35km from Warsaw == By Train == Warsaw can be reached by direct trains from Berlin, Prague and Vienna. Polish Railways schedule is available here: [http://rozklad-pkp.pl/bin/query.exe/en? PKP]. The main station is called Warszawa Centralna. = Workshop Venue = '''Astronomical Observatory of the University of Warsaw''' (in Polish: ''Obserwatorium Astronomiczne Uniwersytetu Warszawskiego'' [https://www.howtopronounce.com/polish/obserwatorium-astronomiczne/ listen]) Address: Aleje Ujazdowskie 4 00-478 Warszawa [https://goo.gl/maps/vDe55iV68hR2 Google map] The Observatory is located together with the Botanic Garden (the same entrance from the street). For public transport itineraries check [http://warszawa.jakdojade.pl/?locale=en warszawa.jakdojade.pl]. Example route to the Workshop venue from the Chopin Airport: [https://jakdojade.pl/warszawa/trasa/z--Warsaw-Chopin-Airport--do--Aleje-Ujazdowskie-4?fn=Warsaw%20Chopin%20Airport&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.17135:20.97239&ft=LOCATION_TYPE_POI&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] The nearest bus stop to the Observatory is called ''Plac na Rozdrozu'' ([https://www.howtopronounce.com/polish/plac-na-rozdrozu/ pronunciation]). From Chopin Airport there is a direct bus no 188, reaching Plac na Rozdrozu in 40 mins. From there it is a 5 minute walk South to the Observatory (will be located on the left). From Modlin Airport the best option is to use [https://www.modlinbus.com/ Modlin Bus] to reach Warsaw City Centre. From there you can either use trams (4, 18, 35) to Plac Unii Lubelskiej [https://jakdojade.pl/warszawa/trasa/z--CENTRUM--do--Aleje-Ujazdowskie-4?fn=CENTRUM&tn=Aleje%20Ujazdowskie%204&tc=52.216796:21.026473&fc=52.23124:21.01015&fsn=CENTRUM&ft=LOCATION_TYPE_STOP&tt=LOCATION_TYPE_ADDRESS&d=27.09.17&h=10:14&aro=1&t=1&rc=3&ri=1&r=0] or Metro M1 line, one stop to Politechnika, and then walk for about 10 mins. = Accommodation = Here is the list of hotels in the city centre and closer to the Observatory: * [http://hamptoninn3.hilton.com/en/hotels/poland/hampton-by-hilton-warsaw-city-centre-WAWCTHX/index.html Hampton by Hilton] * [http://www.novotel.com/gb/hotel-3383-novotel-warszawa-centrum/index.shtml Novotel Warszawa Centrum] * [http://www.hotelmdm.com.pl/ MDM City Centre] * [http://www.castleinn.pl/?lang=en Castle Inn] * [http://www.gromada.pl/en/sportal/hotels/hotel.php?HotelID=1125480&_PageID=26311 Gromada] * [http://www.hotelmetropol.com.pl/default-en.html Metropol] * [http://www.poloniapalace.com/default-en.html Polonia] * [http://www.accorhotels.com/gb/hotel-3714-ibis-warszawa-stare-miasto-old-town/index.shtml Ibis Stare Miasto] * [http://hotelewam.co.uk/635-hotel-belwederski-warsaw.html Belwederski] the nearest to the Observatory * [http://www.lazienkowski.pl/ Łazienkowski] An alternative is AirBnB, where you can find a small flat for less than 50 euro per night [https://www.airbnb.com/s/Warsaw--Poland/homes?refinements%5B%5D=for_you&allow_override%5B%5D=&children=0&infants=0&adults=2&guests=2&room_types%5B%5D=Entire%20home%2Fapt&checkin=2017-11-28&checkout=2017-12-01&ib=true&ne_lat=52.22098485853037&ne_lng=21.032928295019815&sw_lat=52.20984283248001&sw_lng=21.0177791785037&zoom=15&search_by_map=true&s_tag=cnAYtZa9] Some budget options: * [http://thewarsawhostel.com/index.php/en/ Hostel Warsaw] * [http://www.hostel-helvetia.pl/en Hostel Helvetia ] * [http://www.tamkahostel.com/ Hostel Tamka] 655a500a44b73b5110cdd3e71304e87acbf2e9a2 0 285 2220 2017-09-23T06:38:52Z Gsawgwikiadmin 1 Created page with "<big>'''Registration is now open!'''</big> Please register by 31.October 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] == Participants ==" wikitext text/x-wiki <big>'''Registration is now open!'''</big> Please register by 31.October 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] == Participants == 3202eb921bf59c8eb9cda7fe59441fe140bf5bbf 2225 2220 2017-10-03T05:39:16Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Please register by 12.November 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] == Participants == 61864ceee0b698f8467b29f89932bf3feb6bd5e5 2226 2225 2017-10-03T12:43:18Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Please register by 12.November 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Participants == c742c3b95cb00d7036446206eff05c6fdfdfc0ab 2241 2226 2017-10-10T12:10:23Z Gsawgwikiadmin 1 /* Participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Please register by 12.November 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak 23a438a24466631ac3acdd16e0718767cde2d513 2242 2241 2017-10-11T19:12:19Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''Registration is now open!'''</big> Please register by 12.November 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola 3568e26935c51fbbba315ce583cfbb4fe76c336f 2243 2242 2017-10-11T19:12:59Z Gsawgwikiadmin 1 /* Participants */ wikitext text/x-wiki <big>'''Registration is now open!'''</big> Please register by 12.November 2017. [https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM] Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola cbd8cdd998fd9d50e4c383070929eb5553a934e2 2244 2243 2017-10-11T19:13:52Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola 260d6f2b1953d341a0309bb4dfab118a59f4f142 2245 2244 2017-10-12T09:54:36Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy 44117c92bca75f27a57ba75b24c2f14ae62c588c 2247 2245 2017-10-21T05:39:49Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic c935f5ebf94d2fbe07d025ac6d796ba785edde6b 2248 2247 2017-10-26T05:15:58Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova fe560670c53ce733c1dd89f47bb0597019b0a19f 2249 2248 2017-10-27T14:26:36Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva 29be69055e6511900a694669bba72b06400c3cbe 2250 2249 2017-11-03T11:54:39Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski 8c8b103cfe79b909ed538f9f5577445e3306ae33 2251 2250 2017-11-06T06:43:54Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica e0fe6fd79f83b83077e25364cdcc633f6851b8eb 0 286 2221 2017-09-23T06:51:42Z Gsawgwikiadmin 1 Created page with "Gaia Science Alerts is among the leading transient surveys in the world. It has already discovered more than 3000 transients, among them supernovae, cataclysmic variables, mic..." wikitext text/x-wiki Gaia Science Alerts is among the leading transient surveys in the world. It has already discovered more than 3000 transients, among them supernovae, cataclysmic variables, microlensing events and other rare phenomena. Thanks to the whole-sky coverage, superb photometry and astrometry, on-board spectrographs, it is delivering a large and steady stream of interesting alerts. The Gaia Science Alerts team is making a huge effort to maintain and develop the alerting pipeline and the web-pages for alerts. The scientific outcome of Gaia Science Alerts also relies strongly on the intensive follow-up, carried out by our numerous partners from around the globe. The main goals of the 8th Gaia Science Alerts Workshop are: * update on the Gaia and Gaia Alerts status * talk about recent highlights from Gaia Alerts * organize the follow-up campaigns and scientific goals * maintain the existing connections between the follow-up partners * meet new follow-up partners This year we plan to have a hands-on session on Gaia Alerts follow-up organization. We will learn about and practice with the available tools, developed by the Alerts Team. We will learn how to optimise the observations and how to process them in order to maximise the scientific outcome. 3c264dafc2e4e7be2a892578bee3e9b7e12e881d 6 287 2230 2017-10-10T10:20:23Z Gsawgwikiadmin 1 version 1. of the poster wikitext text/x-wiki version 1. of the poster 23a3362d4fed932d8eec6fb0a7d25d65df541674 0 288 2232 2017-10-10T10:24:07Z Gsawgwikiadmin 1 Created page with "[[File:poster2017|450px|poster2017]] '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG Media:poster2..." wikitext text/x-wiki [[File:poster2017|450px|poster2017]] '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2017.png]] * Poster as a PDF [[Media:poster2017.pdf]] 3c72a7c599e1a78f155404a8c42c4cd505035ed6 2233 2232 2017-10-10T10:24:34Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:poster2017.png|450px|poster2017]] '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2017.png]] * Poster as a PDF [[Media:poster2017.pdf]] 2f73cbed3a099b1e30774ada5b70b0aa4d82f99d 2235 2233 2017-10-10T10:25:59Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:poster2017.png|450px|poster2017]] '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2017.png | here]] * Poster as a PDF [[Media:GaiaAlertsWorkshopPoster2017.pdf | here]] 9a6a395f635d0f92d5e1e1bd9418200ae78a3499 2236 2235 2017-10-10T10:26:27Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:poster2017.png|450px|poster2017]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2017.png | here]] * Poster as a PDF [[Media:GaiaScienceAlertsWorkshopPoster2017.pdf | here]] fb4f14f3e905dedcdfb694b35cab12e3a506db45 2240 2236 2017-10-10T12:08:28Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster2017-small.png|450px|poster2017]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2017.png | here]] * Poster as a PDF [[Media:GaiaScienceAlertsWorkshopPoster2017.pdf | here]] 8942301046c036e8efa93ffab464dd31536505e9 6 289 2234 2017-10-10T10:25:25Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 290 2238 2017-10-10T12:07:22Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 283 2252 2246 2017-11-06T15:50:44Z Gsawgwikiadmin 1 wikitext text/x-wiki '''PRELIMINARY AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 6 December 2017''' |---- |---- |12:00 |'''lunch & registration''' | | |---- |2:00 - 5:00 |first session with coffee break | | |---- |---- |colspan="4"| |---- |colspan="4"|'''Thursday, 7 December 2017''' |---- |---- |09:30 |second session with coffee break | | |---- |13:00 | '''lunch''' | | |---- |14:30 |third session with coffee break | | |---- |19:00 |'''conference dinner''' | | |---- |---- |colspan="4"| |---- |colspan="4"|'''Friday, 8 December 2017''' |---- |---- |09:30 |fourth session with coffee break | | |---- |13:00 |'''lunch''' | | |---- |15:00 | end of the workshop | | |---- c464e507f564590a8b787cfbfd71e9a31d23ab5a 2260 2252 2017-11-17T08:20:26Z Gsawgwikiadmin 1 wikitext text/x-wiki '''PRELIMINARY AGENDA''' {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |colspan="4"| |---- |colspan="4"|'''Wednesday, 6 December 2017''' |---- |---- |12:00 |'''lunch & registration''' | | |---- |2:00 - 5:00 |first session with coffee break | | |---- |---- |colspan="4"| |---- |colspan="4"|'''Thursday, 7 December 2017''' |---- |---- |09:30 |second session with coffee break | | |---- |13:00 | '''lunch''' | | |---- |14:30 |third session with coffee break | | |---- |19:00 |'''conference dinner''' [[Workshop2017:menu | menu]] | | |---- |---- |colspan="4"| |---- |colspan="4"|'''Friday, 8 December 2017''' |---- |---- |09:30 |fourth session with coffee break | | |---- |13:00 |'''lunch''' | | |---- |15:00 | end of the workshop | | |---- b28d15ec124065d8c3b57656c13e68c764fb21d2 2263 2260 2017-11-28T13:41:34Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |TAO Konkoly |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |25 |---- |11:00 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:15 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:30 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |11:45 |Giacomo Cannizzaro |Gaia16aax and other nuclear transients |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Wyn Evans |Microlensing in Gaia |15 |---- |14:15 |Katarzyna Kruszyńska |Microlensing events from Gaia |15 |---- |14:30 |Łukasz Wyrzykowski |OPTICON and its role, results |15 |---- |14:45 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:15 |Arancha Delgado |Gaia Marshall demonstration part 1 |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Krakow |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Greek telescopes |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' | |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 9e5791be9c2a697195a10ead05d02ee5ebf1dea1 2264 2263 2017-11-28T22:13:44Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |25 |---- |11:00 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:15 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:30 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |11:45 |Giacomo Cannizzaro |Gaia16aax and other nuclear transients |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Wyn Evans |Microlensing in Gaia |15 |---- |14:15 |Katarzyna Kruszyńska |Microlensing events from Gaia |15 |---- |14:30 |Łukasz Wyrzykowski |OPTICON and its role, results |15 |---- |14:45 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:15 |Arancha Delgado |Gaia Marshall demonstration part 1 |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Krakow |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Greek telescopes |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' | |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 923f19c6f293644f81a1dfc2246bcf55a9e5f071 2266 2264 2017-11-30T18:04:15Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |15 |---- |14:30 |Łukasz Wyrzykowski |OPTICON and its role, results |30 |---- |14:45 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:15 |Arancha Delgado |Gaia Marshall demonstration part 1 |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Krakow |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Greek telescopes |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' | |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- d0dbc21994a57d237c826b9b35fd01ea6d6fa909 2267 2266 2017-12-04T20:55:50Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |15 |---- |14:30 |Łukasz Wyrzykowski |OPTICON and its role, results |30 |---- |14:45 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:15 |Arancha Delgado |Gaia Marshall demonstration part 1 |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Krakow |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Greek telescopes |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 244e511eead3886e1eb25d7c4d87aa646a949f70 2268 2267 2017-12-05T06:38:06Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |15 |---- |14:30 |Łukasz Wyrzykowski |OPTICON and its role, results |30 |---- |14:45 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:15 |Arancha Delgado |Gaia Marshall demonstration part 1 |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Krakow |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Greek telescopes |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 7093470822f933a7a529ee26f3c068921102f00f 2269 2268 2017-12-05T06:55:22Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Krakow |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 326f3cf158a3045b808147255e626f2b8b1b39bc 2270 2269 2017-12-05T21:28:00Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> '''DRAFT AGENDA''' subject to last-minute changes. {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- aa1d1e6f979387068523b9b027dddc8c0331a924 2271 2270 2017-12-06T10:00:24Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:25 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 7c334bfddcfd1b5cd1f9aa228c11b6916a5e6c14 2273 2271 2017-12-07T08:07:37Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia |15 |---- |11:45 |Mariusz Gromadzki |Nuclear transients from OGLE |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 9e28d353e712f2d1dd3de86ddfc1839797f8bc58 2274 2273 2017-12-07T08:38:52Z Lukasz 2 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Varga-Verebélyi Erika |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- cc8bb76a3ea06dd9daaf26128b755f85fa51b5b9 2275 2274 2017-12-07T09:18:54Z Lukasz 2 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |Thuillot William |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- de0470dd1f928c761973ebc545693f79696975a7 2276 2275 2017-12-07T09:19:25Z Lukasz 2 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |William Thuillot |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:00 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:20 |Łukasz Wyrzykowski |OPTICON and its role, results |20 |---- |14:40 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:10 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:20 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |16:30 |Felice Cusano |Gaia alerts in Loiano |10 |---- |16:40 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |16:50 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:00 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:10 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- c56eb8f23231e27444e31f556fce4ed81476a908 2277 2276 2017-12-07T09:35:20Z Lukasz 2 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory |15 |---- |16:15 |William Thuillot |Solar system object alerts |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- d32b3610c542dad3ba658ead87235be860b80ef3 2278 2277 2018-01-09T21:15:52Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SImonHodgkin.pdf PDF] |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SteveBoudreault.pdf PDF] |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaPakstiene.pdf PDF] |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RobertSzakats.pdf PDF] |15 |---- |16:15 |William Thuillot |Solar system object alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/WhiliamThuillot.pdf PDF] |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/VolodimirTroianskyi.pdf PDF] |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GoranDamljanovic.pdf PDF] |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FraserLewis.pdf PDF] |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MilenaRatajczak.pdf PDF] |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/PawelZielinski.pdf PDF] |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrzejPiascik.pdf PDF] |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/HelenJermak.pdf PDF] |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaVargaVerebelyi.pdf PDF] |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/JozsefVarga.pdf PDF] |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RupakRoy.pdf PDF] |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlexHamanowicz.pdf PDF] |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MariuszGromadzki.pdf PDF] |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ThomasWevers.pdf PDF] |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KirillSokolovsky.pdf PDF] |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TapioPursimo.pdf PDF] |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GrzegorzWiktorowicz.pdf PDF] |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KatarzynaKruszynska.pdf PDF] |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/LukaszWyrzykowski1.pdf PDF] |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ZbyszekKolaczkowski.pdf PDF] |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AranchaDelgado.pdf PDF] |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MeredithMorrell.pdf PDF] |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SebastianKurowski.pdf PDF] |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TadeuszMichalowski.pdf PDF] |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FeliceCusano.pdf PDF] |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RicardoZanmarSanchez.pdf PDF] |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/EmmyParaskeva.pdf PDF] |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlgitaStankeviciute.pdf PDF] |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ViraGodunova.pdf PDF] |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndriiSimon.pdf PDF] |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/DawidMozdzierski.pdf PDF] |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 24f189a13e27d7f259448a155a37b863e00024ff 2279 2278 2018-01-09T21:17:07Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SImonHodgkin.pdf PDF] |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SteveBoudreault.pdf PDF] |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaPakstiene.pdf PDF] |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RobertSzakats.pdf PDF] |15 |---- |16:15 |William Thuillot |Solar system object alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/WhiliamThuillot.pdf PDF] |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/VolodimirTroianskyi.pdf PDF] |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GoranDamljanovic.pdf PDF] |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FraserLewis.pdf PDF] |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MilenaRatajczak.pdf PDF] |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/PawelZielinski.pdf PDF] |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrzejPiascik.pdf PDF] |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/HelenJermak.pdf PDF] |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaVargaVerebelyi.pdf PDF] |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/JozsefVarga.pdf PDF] |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RupakRoy.pdf PDF] |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlexHamanowicz.pdf PDF] |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MariuszGromadzki.pdf PDF] |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ThomasWevers.pdf PDF] |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KirillSokolovsky.pdf PDF] |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TapioPursimo.pdf PDF] |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GrzegorzWiktorowicz.pdf PDF] |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KatarzynaKruszynska.pdf PDF] |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/LukaszWyrzykowski1.pdf PDF] |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ZbyszekKolaczkowski.pdf PDF] |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AranchaDelgado.pdf PDF] |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MeredithMorrell.pdf PDF] |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SebastianKurowski.pdf PDF] |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TadeuszMichalowski.pdf PDF] |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FeliceCusano.pdf PDF] |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RicardoZanmarSanchez.pdf PDF] |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/EmmyParaskeva.pdf PDF] |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlgitaStankevicuite.pdf PDF] |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ViraGodunova.pdf PDF] |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndriiSimon.pdf PDF] |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/DawidMozdzierski.pdf PDF] |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 6fb135fae6e1d41985b3477cd64b5744c601e4ef 2280 2279 2018-01-09T21:18:17Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SimonHodgkin.pdf PDF] |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SteveBoudreault.pdf PDF] |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaPakstiene.pdf PDF] |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RobertSzakats.pdf PDF] |15 |---- |16:15 |William Thuillot |Solar system object alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/WhiliamThuillot.pdf PDF] |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/VolodimirTroianskyi.pdf PDF] |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GoranDamljanovic.pdf PDF] |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FraserLewis.pdf PDF] |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MilenaRatajczak.pdf PDF] |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/PawelZielinski.pdf PDF] |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrzejPiascik.pdf PDF] |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/HelenJermak.pdf PDF] |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaVargaVerebelyi.pdf PDF] |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/JozsefVarga.pdf PDF] |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RupakRoy.pdf PDF] |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlexHamanowicz.pdf PDF] |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MariuszGromadzki.pdf PDF] |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ThomasWevers.pdf PDF] |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KirillSokolovsky.pdf PDF] |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TapioPursimo.pdf PDF] |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GrzegorzWiktorowicz.pdf PDF] |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KatarzynaKruszynska.pdf PDF] |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/LukaszWyrzykowski1.pdf PDF] |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ZbyszekKolaczkowski.pdf PDF] |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AranchaDelgado.pdf PDF] |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MeredithMorrell.pdf PDF] |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SebastianKurowski.pdf PDF] |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TadeuszMichalowski.pdf PDF] |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FeliceCusano.pdf PDF] |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RicardoZanmarSanchez.pdf PDF] |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/EmmyParaskeva.pdf PDF] |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlgitaStankevicuite.pdf PDF] |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ViraGodunova.pdf PDF] |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndriiSimon.pdf PDF] |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/DawidMozdzierski.pdf PDF] |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 9f85346c5a04b9474026d3afe1b6fe35a528320e 2281 2280 2018-01-09T21:18:43Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SimonHodgkin.pdf PDF] |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SteveBoudreault.pdf PDF] |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaPakstiene.pdf PDF] |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RobertSzakats.pdf PDF] |15 |---- |16:15 |William Thuillot |Solar system object alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/WhiliamThuillot.pdf PDF] |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/VolodimirTroianskyi.pdf PDF] |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GoranDamljanovic.pdf PDF] |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FraserLewis.pdf PDF] |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MilenaRatajczak.pdf PDF] |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/PawelZielinski.pdf PDF] |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrzejPiascik.pdf PDF] |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/HelenJermak.pdf PDF] |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaVargaVerebelyi.pdf PDF] |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/JozsefVarga.pdf PDF] |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RupakRoy.pdf PDF] |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlexHamanowicz.pdf PDF] |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MariuszGromadzki.pdf PDF] |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ThomasWevers.pdf PDF] |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KirillSokolovsky.pdf PDF] |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TapioPursimo.pdf PDF] |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GrzegorzWiktorowicz.pdf PDF] |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KatarzynaKruszynska.pdf PDF] |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/LukaszWyrzykowski1.pdf PDF] |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ZbyszekKolaczkowski.pdf PDF] |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AranchaDelgado.pdf PDF] |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MeredithMorrell.pdf PDF] |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SebastianKurowski.pdf PDF] |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TadeuszMichalowski.pdf PDF] |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FeliceCusano.pdf PDF] |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RicardoZanmarSanchez.pdf PDF] |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/EmmyParaskeva.pdf PDF] |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlgitaStankevicuite.pdf PDF] |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ViraGodunova.pdf PDF] |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrewSimon.pdf PDF] |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/DawidMozdzierski.pdf PDF] |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- c73349d653af54a916a519dcd608188b391ed2c4 2282 2281 2018-01-09T21:19:58Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SimonHodgkin.pdf PDF] |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SteveBoudreault.pdf PDF] |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaPakstiene.pdf PDF] |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RobertSzakats.pdf PDF] |15 |---- |16:15 |William Thuillot |Solar system object alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/WhiliamThuillot.pdf PDF] |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/VolodimirTroianskyi.pdf PDF] |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GoranDamljanovic.pdf PDF] |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FraserLewis.pdf PDF] |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MilenaRatajczak.pdf PDF] |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/PawelZielinski.pdf PDF] |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrzejPiascik.pdf PDF] |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/HelenJermak.pdf PDF] |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaVargaVerebelyi.pdf PDF] |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/JozsefVarga.pdf PDF] |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RupakRoy.pdf PDF] |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlexHamanowicz.pdf PDF] |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MariuszGromadzki.pdf PDF] |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ThomasWevers.pdf PDF] |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KirillSokolovsky.pdf PDF] |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TapioPursimo.pdf PDF] |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GrzegorzWiktorowicz.pdf PDF] |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KatarzynaKruszynska.pdf PDF] |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/LukaszWyrzykowski1.pdf PDF] |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ZbyszekKolaczkowski.pdf PDF] |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AranchaDelgado.pdf PDF] |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MeredithMorrel.pdf PDF] |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SebastianKurowski.pdf PDF] |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TadeuszMichalowski.pdf PDF] |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FeliceCusano.pdf PDF] |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RicardoZanmarSanchez.pdf PDF] |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/EmmyParaskeva.pdf PDF] |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlgitaStankevicuite.pdf PDF] |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ViraGodunova.pdf PDF] |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrewSimon.pdf PDF] |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/DawidMozdzierski.pdf PDF] |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- c7093ece180e973a74eec4630c47beea705b881c 2283 2282 2018-01-09T21:20:22Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>''' Please provide us with your talks as PDF, Keynote, PowerPoint, OpenOffice before your session!'''</big> Abstract Book [[Media:abstract-book.pdf | PDF]] {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- | |'''Wednesday 6.12.2017''' | | |---- |12:00 |'''lunch and registration''' | |120 |---- |14:00 | |''Welcome by the organizers'' |10 |---- |14:10 |Simon Hodgkin |Gaia overview and alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SimonHodgkin.pdf PDF] |50 |---- |15:00 |Steve Boudreault |PLATO Science Flux Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SteveBoudreault.pdf PDF] |15 |---- |15:15 |Erika Pakstiene |First results of spectroscopic and photometric survey of the northern sky at Moletai AO for the PLATO 2.0 input catalog [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaPakstiene.pdf PDF] |15 |---- |15:30 |'''coffee break''' | |30 |---- |16:00 |Róbert Szakáts |Observations of transient astrophysical objects at Konkoly Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RobertSzakats.pdf PDF] |15 |---- |16:15 |William Thuillot |Solar system object alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/WhiliamThuillot.pdf PDF] |15 |---- |16:30 |Volodymyr Troianskyi |Discovery of the small Solar system bodies with OMT-800 telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/VolodimirTroianskyi.pdf PDF] |10 |---- |16:40 |Goran Damljanovic |Serbian-Bulgarian mini-network telescopes and Gaia-FUN-TO during 2017 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GoranDamljanovic.pdf PDF] |10 |---- |16:50 |Fraser Lewis |Linking Gaia Alerts, supernovae and education [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FraserLewis.pdf PDF] |15 |---- |17:05 |''end of day 1'' | | |---- | |'''Thursday 7.12.2017''' | | |---- |09:15 |Milena Ratajczak |Project Solaris [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MilenaRatajczak.pdf PDF] |15 |---- |09:30 |Pawel Zielinski |Search for young transiting exoplanets within YETI project [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/PawelZielinski.pdf PDF] |15 |---- |09:45 |Andrzej Piascik |Gaia Target Selection on the Liverpool Telescope - Patterns in Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrzejPiascik.pdf PDF] |15 |---- |10:00 |Helen Jermak |MOPTOP — The New Polarimeter for the LT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/HelenJermak.pdf PDF] |15 |---- |10:15 |Erika Varga-Verebélyi |Gaia Photometric Science Alerts for Variable Young Stellar Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ErikaVargaVerebelyi.pdf PDF] |10 |---- |10:25 |Jozsef Varga |Classification of young stellar objects among GAIA alert candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/JozsefVarga.pdf PDF] |10 |---- |10:35 |'''coffee break''' | |40 |---- |11:15 |Rupak Roy |Transients near the centers of the galaxies [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RupakRoy.pdf PDF] |15 |---- |11:30 |Aleksandra Hamanowicz |Nuclear transients from Gaia and OGLE [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlexHamanowicz.pdf PDF] |15 |---- |11:45 |Mariusz Gromadzki |Highlights on Warsaw nuclear transients search [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MariuszGromadzki.pdf PDF] |15 |---- |12:00 |Thomas Wevers |Searching for fast Gaia transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ThomasWevers.pdf PDF] |15 |---- |12:15 |Kirill Sokolovsky |ASASSN-17gs -- awakening of a dormant blazar by a tidal disruption event? [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KirillSokolovsky.pdf PDF] |15 |---- |12:30 |Tapio Pursimo |Optical follow-up observations of Fermi LAT blazars and NOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TapioPursimo.pdf PDF] |15 |---- |12:45 |Grzegorz Wiktorowicz |Black holes as microlenses in the Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/GrzegorzWiktorowicz.pdf PDF] |15 |---- |13:00 |'''lunch break''' | |60 |---- |14:30 |Katarzyna Kruszyńska |Microlensing events from Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/KatarzynaKruszynska.pdf PDF] |20 |---- |14:50 |Łukasz Wyrzykowski |OPTICON and its role, results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/LukaszWyrzykowski1.pdf PDF] |15 |---- |15:05 |Zbyszek Kołaczkowski, Kris Rybicki,Paweł Zieliński |Calibration Server 2.0 beta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ZbyszekKolaczkowski.pdf PDF] |30 |---- |15:35 |'''coffee break''' | |45 |---- |16:10 |Arancha Delgado |Gaia Marshall demonstration part 1 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AranchaDelgado.pdf PDF] |20 |---- |16:30 |Meredith Morrell |PIRATE and Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/MeredithMorel.pdf PDF] |10 |---- |16:40 |Sebastian Kurowski |Photometric measurements from Cracow Observatory - instruments, software & results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/SebastianKurowski.pdf PDF] |10 |---- |16:50 |Tadeusz Michałowski |PST2 - Poznań telescope in Arizona [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/TadeuszMichalowski.pdf PDF] |10 |---- |17:00 |Felice Cusano |Gaia alerts in Loiano [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/FeliceCusano.pdf PDF] |10 |---- |17:10 |Ricardo Zanmar Sanchez |Follow-up from Sicily [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/RicardoZanmarSanchez.pdf PDF] |10 |---- |17:20 |Emmy Paraskeva |Gaia transient follow-up from the National Observatory of Athens [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/EmmyParaskeva.pdf PDF] |10 |---- |17:30 |Algita Stankevičiūtė |Astronomical activities in Lithuania [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AlgitaStankevicuite.pdf PDF] |10 |---- |17:40 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |''cafe Flora, Al. Ujazdowskie 4'' |[[Workshop2017:menu|MENU]] |---- | |'''Friday 8.12.2017''' | | |---- |09:15 |Vira Godunova |Observations of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/ViraGodunova.pdf PDF] |10 |---- |09:25 |Andrii Simon |Observational research at the Lisnyky observatory near Kyiv [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/AndrewSimon.pdf PDF] |10 |---- |09:35 |Dawid Moździerski |Białków Observatory - indispensability of small ground-based telescopes in the era of satellite observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2017/slides/DawidMozdzierski.pdf PDF] |10 |---- |09:45 |Arancha Delgado |hands-on with the new Marshall |45 |---- |10:30 |'''coffee break''' | |30 |---- |11:00 |Łukasz Wyrzykowski |hands-on with the old Calibration Server |45 |---- |11:45 |All |discussion and summary |45 |---- |12:30 |'''lunch break''' | |90 |---- |14:00 |''end of day 3'' | | |---- 6d7ba0b7c480ffa53e99fa8f1f429b5bb3084987 0 285 2253 2251 2017-11-07T12:28:31Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska c11774e73cb19f83ccb21bda8ac0bc799701398e 2254 2253 2017-11-07T12:31:07Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Djouhri Naoual # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska 65a24be22a3edeb629ed999d3b89eb5c54472d0e 2255 2254 2017-11-09T11:50:28Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Djouhri Naoual # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis a9e534dd749ea83bea170ccdafb8953f5489da6f 2256 2255 2017-11-09T15:50:18Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Djouhri Naoual # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis # Zbyszek Kolaczkowski 5ab2042db78051aeddb719e2545978ba7c64975a 2257 2256 2017-11-14T14:39:01Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Djouhri Naoual # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis # Zbyszek Kolaczkowski # Andrii Simon # Dawid Mozdzierski # Andrzej Piascik # Jozsef Varga # Steve Fossey # Lukasz Wyrzykowski # Kris Rybicki 42abe43a3856ccc6e279c0d69dbae0d43c974d71 2258 2257 2017-11-16T15:40:13Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 12.November 2017. <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis # Zbyszek Kolaczkowski # Andrii Simon # Dawid Mozdzierski # Andrzej Piascik # Jozsef Varga # Steve Fossey # Lukasz Wyrzykowski # Kris Rybicki # Simon Hodgkin # Elme Breedt # Arancha Delgado efc1684a2428ca1b03f67be6c544203c811b9fcc 2259 2258 2017-11-17T07:26:35Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now closed</big> == <!-- <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> --> If you are still desperate to join our meeting, please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) as soon as possible. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis # Zbyszek Kolaczkowski # Andrii Simon # Dawid Mozdzierski # Andrzej Piascik # Jozsef Varga # Steve Fossey # Lukasz Wyrzykowski # Kris Rybicki # Simon Hodgkin # Elme Breedt # Arancha Delgado 71487def59b5e9c563a00da2381b1569765be17f 2262 2259 2017-11-20T11:57:10Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now closed</big> == <!-- <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> --> If you are still desperate to join our meeting, please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) as soon as possible. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis # Zbyszek Kolaczkowski # Andrii Simon # Dawid Mozdzierski # Andrzej Piascik # Jozsef Varga # Steve Fossey # Lukasz Wyrzykowski # Kris Rybicki # Simon Hodgkin # Elme Breedt # Arancha Delgado # Volodymyr Troianskyi 62bb66fa2ae7e1b084746b397f648877db565c2b 2265 2262 2017-11-28T22:16:55Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now closed</big> == <!-- <big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big> --> If you are still desperate to join our meeting, please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) as soon as possible. == Registered participants == # Felice Cusano # Mariusz Gromadzki # Ricardo Zanmar Sanchez # Thomas Wevers # Aleksandra Hamanowicz # Giacomo Cannizzaro # Helen Jermak # Staszek Zola # Rupak Roy # William Thuillot # Milena Ratajczak # Pawel Zielinski # Erika Pakstiene # Meredith Morrell # Steve Boudreault # Peter McGill # Goran Damljanovic # Wyn Evans # Vira Godunova # Emma Paraskeva # Algita Stankeviciute # Sebastian Kurowski # Tapio Pursimo # Kirill Sokolovsky # Nada Ihanec # Szymon Zywica # Robert Szakats # Katarzyna Kruszynska # Erika Varga-Verebélyi # Fraser Lewis # Zbyszek Kolaczkowski # Andrii Simon # Dawid Mozdzierski # Andrzej Piascik # Jozsef Varga # Steve Fossey # Lukasz Wyrzykowski # Kris Rybicki # Simon Hodgkin # Arancha Delgado # Volodymyr Troianskyi # Katarzyna Drozd # Grzegorz Wiktorowicz # Tadeusz Michałowski # Barbara Handzlik fb808262b2524035d035fdf805879ea9cfb47bce 0 291 2261 2017-11-17T08:29:21Z Gsawgwikiadmin 1 Created page with "==Place== Flora Caffee, next to the Observatory. ==Time== Thursday, 7.Dec, 19:00 ==Menu== ==== Starters ==== (all will be available for everyone) Warm: Blini with salmon (..." wikitext text/x-wiki ==Place== Flora Caffee, next to the Observatory. ==Time== Thursday, 7.Dec, 19:00 ==Menu== ==== Starters ==== (all will be available for everyone) Warm: Blini with salmon (Russian pancakes) Cold: Marinated pears with cheese selection (V) Eggs in mayo (V) Herring with apple and cream Grilled eggplant filled with nutty paste (V) ==== Soup ==== Zurek with egg (white borsch) (V) ==== Main ==== Duck baked with potatoes and apples or Lecho with rice (V) ==== Desert ==== Selection of traditional Polish cakes (Christmas cakes): cheescake, poppy-seed cake. Tea, coffee, water available anytime. Selection of white and red wines. Espresso coffee available for purchase in the bar. 38134b32b779ec40a6862f7687b016ca1c4464b6 6 292 2272 2017-12-06T10:00:43Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 1 2284 2210 2018-04-18T15:17:02Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava, Slovenia, 8-10 October 2018]]</Big>''' </center> ---- <center> [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 5b0c74d39fc195a7cd39277b0ff4de477557b29a 0 293 2285 2018-04-18T15:19:01Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in Workshop2018:logistics | Vipava/Slove..." wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' SCOPE Please fill the [[workshop2018:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) 56c4c826f6c25a484b4ec2d77fe4da41d0fd62fe 2290 2285 2018-04-19T12:36:25Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' SCOPE Please fill the [[workshop2018:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) 0348658b720f4dd920653a4610834d6d6da6289f 2293 2290 2018-04-20T07:25:55Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' The main goals of this year's workshop are: - update on the Gaia mission - update on the improvements in the Gaia Alerts -Gaia Alerts highlights - machine-learning classification of transients - Gaia Alerts and DR2 - new photometric calibration server - organization of the follow-up ---- Please fill the [[workshop2018:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) 4efe959a7eff4efb98703d33cc0c549e6b2cb428 2294 2293 2018-04-20T07:26:22Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights * machine-learning classification of transients * Gaia Alerts and DR2 * new photometric calibration server * organization of the follow-up ---- Please fill the [[workshop2018:registration|registration form]] and provide your case why do you want to attend the workshop. ---- ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) cf5984f5785703268d5591f7a4909feaa50d3442 0 294 2286 2018-04-18T15:20:33Z Gsawgwikiadmin 1 Created page with "== <big>Registration is now open!</big> == Please register by 1.September 2018. <!--<big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big>--> Note, th..." wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 1.September 2018. <!--<big>'''[https://goo.gl/forms/JKxzyEAArySUhyy82 REGISTRATION FORM]'''</big>--> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request. == Registered participants == # 9e52893921d986c4522fa901995c32579a4ccb5d 2291 2286 2018-04-19T12:49:25Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 1.September 2018. <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request by 1. August 2018. == Registered participants == # ce193dd78f9cce678df7e0ae8695c18c9815ccd7 8 3 2287 2211 2018-04-19T12:31:43Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2018 **workshop2018:main|Main Workshop Page **workshop2018:rationale|Rationale **workshop2018:agenda|Program **workshop2018:registration|Participants and Registration **workshop2018:logistics|Logistics *workshop 2017 **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 473df1e799e1564693e0acfd6e92e3d1043a5756 0 295 2288 2018-04-19T12:33:50Z Gsawgwikiadmin 1 Created page with "= Travel Info = == By Air == == By Train == = Workshop Venue = Address: University of Nova Gorica, Glavni trg 8, Vipava, Slovenia [https://www.google.si/maps/place/Unive..." wikitext text/x-wiki = Travel Info = == By Air == == By Train == = Workshop Venue = Address: University of Nova Gorica, Glavni trg 8, Vipava, Slovenia [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] = Accommodation = b0cbe3016fe0898063589a0db9fbac2200c88fde 2289 2288 2018-04-19T12:34:13Z Gsawgwikiadmin 1 wikitext text/x-wiki = Travel Info = == By Air == == By Train == = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia Address: University of Nova Gorica, Glavni trg 8, Vipava, Slovenia [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] = Accommodation = 229644c681864e1610d178e46dbbaf3c918fff40 2295 2289 2018-04-23T22:54:36Z Nada.ihanec 43 wikitext text/x-wiki = Travel Info = The workshop will take place at Lanthieri Manor in Vipava, Slovenia. Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capitol Ljubljana. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''Ljubljana LJU''' [https://www.adria.si/en/flights-and-destinations/] It is connected to most major cities over Europe. There are also two Italian airports that we recommend: '''Trieste (TRS)''' [https://triesteairport.it/en/airport/] which is actually closer to Vipava than Slovenian one and is bigger and has more connections. '''Treviso (TSF)''' [http://www.trevisoairport.it/en/] Car service '''GoOpti''' [https://www.goopti.com/en/] will take you from any airport to Ljubljana. == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here: Slovenske Železnice [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad] Slovenian railways schedule can be found here: [http://www.slo-zeleznice.si/en/] == By Bus == There is also possibility of arriving with buss. [https://www.flixbus.co.uk/] = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia Address: University of Nova Gorica, Glavni trg 8, Vipava, Slovenia [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] = Accommodation = 0ff3e0561375e01eb0066e90591e61c30c7b9631 2296 2295 2018-05-09T19:36:15Z Nada.ihanec 43 wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capitol Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your choosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also possibility of arriving with [https://www.flixbus.co.uk/ buss]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = d452d14b85c21f569d20409f3ddfdc2cce883053 2297 2296 2018-05-09T19:55:13Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capitol Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your choosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also possibility of arriving with [https://www.flixbus.co.uk/ buss]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: *[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] *[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] *[http://www.apartmaji-koren.com/english/english.html David Koren apartments] *[https://turizem-nahribu.com/en/sobe/ Na hribu] *[http://www.majerija.si/en/accommodation/ Majerija] We also urge you to book it in advance and not in the last minute due to the small capacities. ---- There will be '''organized buss transfer''' every day from the above accommodations to Lanthieri mansion. ---- 99e8a26f9f369aa5a8471f87d82770b5e94e5bfc 2298 2297 2018-05-09T20:04:49Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capitol Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your choosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also possibility of arriving with [https://www.flixbus.co.uk/ buss]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: *[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] *[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] *[http://www.apartmaji-koren.com/english/english.html David Koren apartments] *[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] *[https://turizem-nahribu.com/en/sobe/ Na hribu] *[http://www.majerija.si/en/accommodation/ Majerija] We also urge you to book it in advance and not in the last minute due to the small capacities. ---- There will be '''organized buss transfer''' every day from the above accommodations to Lanthieri mansion. ---- An alternative is also [https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB] 175de8a0a781e3bab7bcff7ccaee1a6861e00546 2299 2298 2018-05-09T20:16:28Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capitol Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your choosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also possibility of arriving with [https://www.flixbus.co.uk/ buss]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: *[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] *[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] *[http://www.apartmaji-koren.com/english/english.html David Koren apartments] *[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] *[https://turizem-nahribu.com/en/sobe/ Na hribu] *[http://www.majerija.si/en/accommodation/ Majerija] We also urge you to book it in advance and not in the last minute due to the small capacities. ---- There will be '''organized buss transfer''' every day from the ''above'' accommodations to Lanthieri mansion. ---- '''An alternative is also [https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 92521fac1926f1204fdf0b4f99beca223f8c0572 2300 2299 2018-05-09T20:17:11Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capitol Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your choosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also possibility of arriving with [https://www.flixbus.co.uk/ buss]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: *[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] *[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] *[http://www.apartmaji-koren.com/english/english.html David Koren apartments] *[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] *[https://turizem-nahribu.com/en/sobe/ Na hribu] *[http://www.majerija.si/en/accommodation/ Majerija] We also urge you to book it in advance and not in the last minute due to the small capacities. ---- There will be '''organized buss transfer''' every day from the ''above'' accommodations to Lanthieri mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 58b4ac4a9e6331a4e678e3b5a4f537e44e757881 2301 2300 2018-05-10T06:08:28Z Gsawgwikiadmin 1 wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your chosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: *[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] *[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] *[http://www.apartmaji-koren.com/english/english.html David Koren apartments] *[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] *[https://turizem-nahribu.com/en/sobe/ Na hribu] *[http://www.majerija.si/en/accommodation/ Majerija] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the ''above'' accommodations to Lanthieri mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 94310c41cc2a95c19b1fe3b923d2cad753530f11 0 296 2292 2018-04-20T07:23:19Z Gsawgwikiadmin 1 Created page with "Gaia is now a well established and leading transient mission. It discovers nearly 2000 objects a year from all over the sky, down to about 20 mag, covering all possible classe..." wikitext text/x-wiki Gaia is now a well established and leading transient mission. It discovers nearly 2000 objects a year from all over the sky, down to about 20 mag, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing and tidal disruption events. The discovery machine within Gaia is still evolving and year 2018 brings many significant improvements and changes in the Gaia Alerts system and its operation. With the second Gaia data release (GDR2), the Gaia-computed distances to a billion of stars will change the landscape of transient science. In particular, the progenitors of Galactic transients will now have their distances measured, hence absolute magnitudes can be computed, aiding the classification and enabling discoveries of rare and unique classes of transients, e.g., AM CVn. Machine learning-supported classification of transients based on Gaia data, in particular, its low-resolution BPRP spectra available for every observation, will boost the success rate in recognising common types of transients as well as the most unusual ones. The follow-up observations from the ground will be able to automatise their photometric data processing with a new and improved Calibration Server. This will also allow more amateur observers to take part in the observations of Gaia alerts. The 2018 Gaia Alerts Workshop, the 9th in the series, will again be an opportunity to learn about Gaia and Gaia Alerts, to meet people behind the pipelines and web pages, to find out about most recent scientific highlights from Gaia Alerts and to discuss the scientific potential of this programme. f362809fc67726e1523410fb7ca375dff43d0809 0 295 2302 2301 2018-05-10T10:40:28Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your chosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: 1.[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] 2.[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] 3.[https://turizem-nahribu.com/en/sobe/ Na hribu] 4.[http://www.majerija.si/en/accommodation/ Majerija] 5.[http://www.apartmaji-koren.com/english/english.html David Koren apartments] 6.[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 63b09684b53ec9fc68db6b3c676a0ca6830267f5 2303 2302 2018-05-10T10:41:10Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use GoOpti for transfer from your chosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: * 1.[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] * 2.[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] * 3.[https://turizem-nahribu.com/en/sobe/ Na hribu] * 4.[http://www.majerija.si/en/accommodation/ Majerija] * 5.[http://www.apartmaji-koren.com/english/english.html David Koren apartments] * 6.[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 22ef91d258f0ff5465aaeacf4eb04a3ef586b12c 2304 2303 2018-05-10T11:03:48Z Nada.ihanec 43 wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also two Italian airports that we recommend: ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use '''GoOpti''' for transfer from your chosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: * 1.[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] * 2.[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] * 3.[https://turizem-nahribu.com/en/sobe/ Na hribu] * 4.[http://www.majerija.si/en/accommodation/ Majerija] * 5.[http://www.apartmaji-koren.com/english/english.html David Koren apartments] * 6.[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 67a4c5f19be2af840b1eec77b4c0802539efa7b4 2305 2304 2018-05-10T11:04:40Z Nada.ihanec 43 /* By Air */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- We recommend that you use '''GoOpti''' for transfer from your chosen airport. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: * 1.[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] * 2.[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] * 3.[https://turizem-nahribu.com/en/sobe/ Na hribu] * 4.[http://www.majerija.si/en/accommodation/ Majerija] * 5.[http://www.apartmaji-koren.com/english/english.html David Koren apartments] * 6.[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' bf4987624a8473adac81da4a68b64a5c86a0ec31 2306 2305 2018-05-10T11:14:51Z Nada.ihanec 43 /* By Air */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- Here are some options for transfer from your chosen airport to Vipava or your place of stay: ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: * 1.[http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] * 2.[https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] * 3.[https://turizem-nahribu.com/en/sobe/ Na hribu] * 4.[http://www.majerija.si/en/accommodation/ Majerija] * 5.[http://www.apartmaji-koren.com/english/english.html David Koren apartments] * 6.[http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 0bb6dffd09fc2e680af4f38b63376fbe3b7207d3 2307 2306 2018-05-10T11:18:25Z Nada.ihanec 43 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. New York Times article about the region: [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html] = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- Here are some options for transfer from your chosen airport to Vipava or your place of stay: ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] # [https://turizem-nahribu.com/en/sobe/ Na hribu] # [http://www.majerija.si/en/accommodation/ Majerija] # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 3b2c5e35a3910cde8e0b37990ebd93e10ff7ea95 2312 2307 2018-05-22T11:41:22Z Nada.ihanec 43 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vivava valley as one of the [https://www.lonelyplanet.com/best-in-europetop 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- Here are some options for transfer from your chosen airport to Vipava or your place of stay: ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] # [https://turizem-nahribu.com/en/sobe/ Na hribu] # [http://www.majerija.si/en/accommodation/ Majerija] # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 0dcd68b963330609f181c7f41b7b927120800183 2313 2312 2018-05-22T11:41:56Z Nada.ihanec 43 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vivava valley as one of the [https://www.lonelyplanet.com/best-in-europetope 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- Here are some options for transfer from your chosen airport to Vipava or your place of stay: ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] # [https://turizem-nahribu.com/en/sobe/ Na hribu] # [http://www.majerija.si/en/accommodation/ Majerija] # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 4ec3e5c9cf08bdcd77693d30b6fc14c228fd547c 2314 2313 2018-05-22T11:42:36Z Nada.ihanec 43 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vivava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- Here are some options for transfer from your chosen airport to Vipava or your place of stay: ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] # [https://turizem-nahribu.com/en/sobe/ Na hribu] # [http://www.majerija.si/en/accommodation/ Majerija] # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' dc14d9d899e5f7b0acaa11a2623c6ab1faf892f0 2315 2314 2018-05-22T12:06:21Z Nada.ihanec 43 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == Slovenia has one airport near the capitol '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''' It is connected to most major cities over Europe. There are also Italian airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''' which is actually closer to Vipava than Slovenian one and is bigger and has more connections. * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections ---- Here are some options for transfer from your chosen airport to Vipava or your place of stay: ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] # [https://turizem-nahribu.com/en/sobe/ Na hribu] # [http://www.majerija.si/en/accommodation/ Majerija] # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' 7f8bf6234e1c3d3260c77b56d73e9698b6fdfa1f 2316 2315 2018-06-01T15:48:58Z Nada.ihanec 43 wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The best way to travel from your chosen airport to any given address is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) Arriving/going to Trieste (central station) there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] # [https://turizem-nahribu.com/en/sobe/ Na hribu] # [http://www.majerija.si/en/accommodation/ Majerija] # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] We also urge you to book it in advance and not at the last minute due to the small capacities. ---- There will be '''organized bus transfer''' every day from the accommodations numbered 1-4 to Lanthieri mansion. However 5. and 6. are a walking distance from the mansion. ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' b306f265aa8905fcfc0b4bd1519aa3401efa54f0 2317 2316 2018-06-11T21:11:28Z Nada.ihanec 43 wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to[https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . e5828912ad006952333083d009c0444f1b3dd9a5 2320 2317 2018-06-11T22:02:19Z Nada.ihanec 43 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = [[File:lanth.jpg|right|300 px | Main entrance to Lanthieri Mansion]] Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to[https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . c352729051ddd035bae5f48f1e7b2ebe503dda1e 2321 2320 2018-06-11T22:03:05Z Nada.ihanec 43 /* Social Program */ wikitext text/x-wiki = Workshop Venue = [[File:lanth.jpg|right|300 px | Main entrance to Lanthieri Mansion]] Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Info = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == There is also a possibility for arriving with [https://www.flixbus.co.uk/ bus]. http://www.ap-ljubljana.si/en/ lists all bus connections inside Slovenia (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to [https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . d952cd879ced8d5fab80b2011317be3dff47e627 2322 2321 2018-06-11T22:35:29Z Nada.ihanec 43 /* Travel Info */ wikitext text/x-wiki = Workshop Venue = [[File:lanth.jpg|right|300 px | Main entrance to Lanthieri Mansion]] Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. = Travel Information = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == [https://www.flixbus.co.uk/ Flixbus] connects all major European cities with Ljubljana. ---- There is a bus connection from '''Ljubljana''' to '''Vipava'''. All the informations can be found here: http://www.ap-ljubljana.si/en/ (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to [https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . 8523341f20f083d535e6a949c4f28c0cd2303aca 2323 2322 2018-06-13T13:03:07Z Nada.ihanec 43 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia <html><iframe src="https://www.google.com/maps/embed?pb=!4v1528893590083!6m8!1m7!1sYxEeiRNUSti-t2rSI494nA!2m2!1d45.8455659313778!2d13.96255872562424!3f122.63435973899519!4f-1.0797039501755847!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. <html><iframe width="560" height="315" src="https://www.youtube.com/embed/6kX8rvYokV0" frameborder="0" allow="autoplay; encrypted-media" allowfullscreen></iframe></html> = Travel Information = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] == By Bus == [https://www.flixbus.co.uk/ Flixbus] connects all major European cities with Ljubljana. ---- There is a bus connection from '''Ljubljana''' to '''Vipava'''. All the informations can be found here: http://www.ap-ljubljana.si/en/ (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to [https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . 6a5fd40332c240e45671ac61d70336c5e004166b 2324 2323 2018-06-14T11:32:30Z Nada.ihanec 43 /* By Train */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia <html><iframe src="https://www.google.com/maps/embed?pb=!4v1528893590083!6m8!1m7!1sYxEeiRNUSti-t2rSI494nA!2m2!1d45.8455659313778!2d13.96255872562424!3f122.63435973899519!4f-1.0797039501755847!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. <html><iframe width="560" height="315" src="https://www.youtube.com/embed/6kX8rvYokV0" frameborder="0" allow="autoplay; encrypted-media" allowfullscreen></iframe></html> = Travel Information = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] Slovenian railways schedule can be found here [http://www.slo-zeleznice.si/en/ slo-zelezice] ---- There is a bus connection from '''Ljubljana''' to '''Vipava'''. All the informations can be found here: http://www.ap-ljubljana.si/en/ (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) == By Bus == [https://www.flixbus.co.uk/ Flixbus] connects all major European cities with Ljubljana. ---- There is a bus connection from '''Ljubljana''' to '''Vipava'''. All the informations can be found here: http://www.ap-ljubljana.si/en/ (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to [https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . c96d138237d24f232b098728f125bce9d030445e 2325 2324 2018-06-14T11:43:12Z Nada.ihanec 43 /* By Train */ wikitext text/x-wiki = Workshop Venue = Lanthieri Mansion, Vipava, Slovenia [https://www.wmf.org/project/lanthieri-manor] '''Address:''' [https://www.google.si/maps/place/Univerza+v+Novi+Gorici/@45.8454874,13.9628235,15z/data=!4m5!3m4!1s0x0:0x3bec7ba42cc0aac8!8m2!3d45.8454874!4d13.9628235] University of Nova Gorica, Glavni trg 8, Vipava, Slovenia <html><iframe src="https://www.google.com/maps/embed?pb=!4v1528893590083!6m8!1m7!1sYxEeiRNUSti-t2rSI494nA!2m2!1d45.8455659313778!2d13.96255872562424!3f122.63435973899519!4f-1.0797039501755847!5f0.7820865974627469" width="600" height="450" frameborder="0" style="border:0" allowfullscreen></iframe></html> ---- Vipava is a small town in western Slovenia. It is approximately 80 kilometers west from the capital Ljubljana. The [https://www.youtube.com/watch?v=6kX8rvYokV0 valley of Vipava river] is known for its natural beauty and wine production. There are many hiking possibilities in the near by hills and it is a home to some of the most beautiful caves (e.g. [https://www.postojnska-jama.eu/en/ Postojna], [http://www.park-skocjanske-jame.si//en/read/the-skocjan-caves/explore-the-caves Skocjan]) in the region. ''New York Times'' [http://www.nytimes.com/2014/06/22/travel/with-wind-calm-serenity-in-slovenia.html article] about the region. ''Lonely Planet'' put Vipava valley as one of the [https://www.lonelyplanet.com/best-in-europe 10 essential destinations in Europe this year]. <html><iframe width="560" height="315" src="https://www.youtube.com/embed/6kX8rvYokV0" frameborder="0" allow="autoplay; encrypted-media" allowfullscreen></iframe></html> = Travel Information = The workshop will take place at Lanthieri Mansion in Vipava, Slovenia. '''Traveling to Slovenia:''' == By Air == The closest airports that we recommend: * ''' [https://triesteairport.it/en/airport/ Trieste (TRS)] ''': the closest to Vipava * ''' [http://www.trevisoairport.it/en/ Treviso (TSF)] ''' * ''' [http://www.veniceairport.it/en/ Venice airport Marco Polo]''': offers low fare easy jet flights in addition to many standard airline connections * '''[https://www.adria.si/en/flights-and-destinations/ Ljubljana LJU]''': Slovenian airport, is connected to most major cities over Europe. ---- The '''best way to travel from your chosen airport to any given address''' is '''GoOpti''', which we highly recommend. ''' [https://www.goopti.com/en/ GoOpti]''' company offers shared and private rides connecting all the airports to the address of your choosing. This service can only be booked through their website. We urge you to book it as soon as possible, since it will be cheaper this way. Upon filling in your chosen destinations and time of the departure you will then have an opportunity to choose between given pick-up times. You will receive conformation about booking immediately on your email and then a massage at least a day before the departure with the exact hour of departure. It might also be a good idea to '''rent a car once arrived at the airport''' for those who like being more independent. Keep in mind that Vipava is 1-2 hour car drive away from all mentioned airports. It is also possible (but less convenient) to use a '''train+bus to get from the airport''' to Vipava: Train schedule for Italian trains (connecting Venice - Trieste - Gorizia can be found here: [http://www.trenitalia.com/trenitalia21.html train schedule]) For getting from Trieste airport to Trieste central station there are two options: * Train: [https://www.trenitalia.it tickets and schedule] * [https://www.aptgorizia.it/ProxyVFS.axd/allegato1,orig/r13648/APT-Collegamenti-Aeroporto-FVG-Inverno-2014-15-ediz_2-pdf?ext=.pdf 51 bus ] Connecting the Trieste (central station) and Vipava there is a bus, once per day [https://www.autostazionetrieste.it/en-us Trieste - Vipava] (14:45 Trieste - 16:19 Vipava and 05:36 Vipava - 7:13 Trieste). == By Train == Ljubljana can be reached by trains from some cities around Europe. More information about this can be found here [http://www.slo-zeleznice.si/en/passenger-transport/travelling-abroad Slovenske Železnice] ---- Vipava doesn't have a train station, so the easiest way to come to Vipava from Ljubljana is either with a '''bus''' or again one can use '''GoOpti'''. There is a bus connection from '''Ljubljana''' to '''Vipava'''. All the informations can be found here: http://www.ap-ljubljana.si/en/ (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) == By Bus == [https://www.flixbus.co.uk/ Flixbus] connects all major European cities with Ljubljana. ---- There is a bus connection from '''Ljubljana''' to '''Vipava'''. All the informations can be found here: http://www.ap-ljubljana.si/en/ (the relevant bus stations are LJUBLJANA AVTOBUSNA POSTAJA, Nova Gorica, Ajdovščina and Vipava) = Accommodation = We recommend that you choose from one of the following accommodations: # [http://www.hotelgoldclub.eu/en/hotel/ GOLD CLUB Ajdovščina] (25 rooms on hold for workshop participants until Aug 10th, 2018, single: 40 Eu/night, double: 75 Eu/night for 2 persons, including breakfast) # [https://turizem-nahribu.com/en/sobe/ Na hribu] (10 rooms, single: 25Eu/night, double: 34 Eu/night for 2 persons, minimum stay 2 nights) # [http://www.majerija.si/en/accommodation/ Majerija] (4 rooms, single room 73 Eu/night, double 98 Eu/night for 2 persons, including breakfast) # [https://www.hostel-ajdovscina.si/accommodation/ The Youth Hostel Ajdovščina] (three 4-beds rooms, one 6-beds, one 8-beds and one 24 beds room, 18-21 Eu/night) # [http://www.apartmaji-koren.com/english/english.html David Koren apartments] (4 apartments, 3 rooms, in Vipava) # [http://apartment-thomas-si.book.direct/en-gb/ Apartment Thomas] (1 apartment, in Vipava) We urge you to '''book the accommodation as soon as possible''' due to a small number of available rooms. Please consider also sharing a room with a colleague. If you decide to stay in one of the above places, please mention at the time of booking that you are attending an astronomical “Gaia workshop” organised by the University of Nova Gorica. In case there are no more available rooms in above accommodations, please, contact us and we will try to find other options. ---- During the workshop there will be '''daily bus transfer organized''' between accommodations numbered 1-4 to the workshop venue (Lanthieri mansion, Vipava). Accommodation 5. and 6. are a walking distance from the workshop venue (Lanthieri mansion, Vipava). ---- An alternative is also '''[https://www.airbnb.com/s/Vipava--Slovenia/homes?refinement_paths%5B%5D=%2Fhomes&query=Vipava%2C%20Slovenia&allow_override%5B%5D=&ne_lat=45.86626001674457&ne_lng=13.986203751997095&sw_lat=45.82503512991585&sw_lng=13.937537751630884&search_by_map=true&zoom=14&s_tag=1cXAv9_s AirBnB]''' = Social Program = For those arriving over the weekend before the workshop, we plan to organize a trip to [https://www.postojnska-jama.eu/en/ Postojna Cave] on Sun, Oct 7th in the afternoon. We plan to have: * a welcome reception in the Lanthieri Mansion on Sun, Oct 7th evening, * a local food+wine tasting in one of the local wineries on Mon, Oct 8th evening, * workshop dinner on Tue, Oct 9th . 0a0bb3f6229affabfc35a02b01524c828937b1cc 6 297 2308 2018-05-21T14:29:09Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 298 2309 2018-05-21T14:29:52Z Gsawgwikiadmin 1 Created page with "[[File:Poster2018-small.png|450px|poster2018]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG..." wikitext text/x-wiki [[File:Poster2018-small.png|450px|poster2018]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2018.png | here]] * Poster as a PDF [[Media:GaiaScienceAlertsWorkshopPoster2018.pdf | here]] 03133e422b96b65231fe5c060660fdb34b4df5a1 6 299 2310 2018-05-21T14:30:09Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 300 2311 2018-05-21T14:30:24Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 301 2318 2018-06-11T21:17:52Z Nada.ihanec 43 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 302 2319 2018-06-11T21:59:31Z Nada.ihanec 43 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 303 2326 2018-08-22T10:07:26Z Gsawgwikiadmin 1 Created page with "The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- Draft agenda (subject to changes): '''Monday 8th O..." wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- Draft agenda (subject to changes): '''Monday 8th October 2018''' <!--- 09:00 - 11:00 registration, coffee 11:00 start of the workshop ---> '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' 2e7e04f5498e573a079d497f8c1fbe2dd5f0719e 2327 2326 2018-08-24T05:59:08Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- Draft agenda (subject to changes): '''Monday 8th October 2018''' 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave 96b89a14c31007b2731b63ceaea35d50bd7eedc5 2332 2327 2018-09-13T06:00:01Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- Draft agenda (subject to changes): '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave a11986bc4d7c27f0204fbe5557ced535295874cf 2335 2332 2018-09-17T11:08:36Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- Draft agenda (subject to changes): '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave bcf25bd1c2608f60d86551a5e49f81b5b59bc59f 2336 2335 2018-09-22T15:58:23Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[agenda-programme.pdf Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave 8c8a4ae6a37ad13dc3960a5c2f15adc2ac170129 2337 2336 2018-09-22T15:58:39Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[file:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave 6deb4e0e56781b43b934814b9e23df83a4e7529d 2339 2337 2018-09-22T15:59:47Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave 8a54c43f09afd14985477cae869700fc5c791578 2340 2339 2018-09-24T16:23:19Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[File:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave fafb15e05ea3071d92659f92fa9266c6d497277b 2341 2340 2018-09-24T16:23:31Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave 8a54c43f09afd14985477cae869700fc5c791578 2343 2341 2018-10-02T10:37:35Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |30 |---- |17:10 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |45 |---- |17:55 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |"Black holes with microlensing | introduction" |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |coffee break | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |lunch break | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |"The importance of Gaia mission for  | |---- |Dark Matter searches" |15 | | |---- |15:10 |coffee break | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |end of day 2 | | |---- |19:00 |workshop dinner |https://gostilna-theodosius.si/ | |---- | |Wednesday 10.10.2018 | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |coffee break | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |end of day 3 | | |---- |12:30 |lunch | | |---- |14:00 |trip to Postojna Cave | | |---- } ea5674d43ac33fdcb0f6ad09d108442a28dbd662 2344 2343 2018-10-02T12:01:24Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |30 |---- |17:10 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |45 |---- |17:55 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''''end of day 2'''' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''''end of day 3'''' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- } c978bf7628bb5351ff45ff5b4477db76e1ab17e3 2345 2344 2018-10-02T12:02:09Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''13:00 lunch and end of the workshop'' optional trip to Postojna Cave {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |30 |---- |17:10 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |45 |---- |17:55 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- } a0ff066db946826b12315139d4dc5c20953ce9bd 2346 2345 2018-10-02T12:03:19Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''title''' |'''name''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |30 |---- |17:10 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |45 |---- |17:55 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- a07d46612dda84370f0a008c9c8568c8c6f2c91e 2347 2346 2018-10-02T12:04:13Z Gsawgwikiadmin 1 /* Detailed programme */ wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |30 |---- |17:10 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |45 |---- |17:55 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- 4ce4468cd2492edf83b08a70d11074953e768d31 2350 2347 2018-10-02T14:41:07Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |17:35 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |25 |---- |18:00 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- c1bb8fb22af30836a656df57ac4ce9a19799ecd8 2351 2350 2018-10-02T14:41:26Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |25 |---- |18:00 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- d255b603466fab6c15cbdd828b197645960d6f4e 0 294 2328 2291 2018-08-28T22:58:56Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 10 September 2018. <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request by 1. August 2018. == Registered participants == # 0d9d34c14c8b7d1b2d26bfb98ad41a62addec0fb 2329 2328 2018-09-11T15:48:52Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 10 September 2018. <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request by 1. August 2018. == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory d41378e7845ea730ddda69dbac508501b05ad13a 2330 2329 2018-09-12T05:01:58Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 10 September 2018. <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request by 1. August 2018. == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory # Giuseppe Leto INAF - Catania Astrophysical Observatory # Ricardo Zanmar Sanchez INAF - OACT # Mariusz Gromadzki Warsaw Astronomical Observatory 6924666deb7b18a7886b253c3bf0c52a8fcbc0f8 2331 2330 2018-09-13T05:56:45Z Gsawgwikiadmin 1 /* Registered participants */ wikitext text/x-wiki == <big>Registration is now open!</big> == Please register by 10 September 2018. <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> Note, there is no registration fee! There will be a possibility for limited financial support. Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) with details of your request by 1. August 2018. == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory # Giuseppe Leto INAF - Catania Astrophysical Observatory # Ricardo Zanmar Sanchez INAF - OACT # Mariusz Gromadzki Warsaw Astronomical Observatory # Laurent Eyer University of Geneva 3e04ee2927f6d63577275bf06435b0ab2e6f8006 2333 2331 2018-09-14T10:57:37Z Gsawgwikiadmin 1 /* Registration is now open! */ wikitext text/x-wiki == <big>Registration is now open!</big> == Registration closed. <!-- <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> --> Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) if you would like to join the meeting at the very last minute! == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory # Giuseppe Leto INAF - Catania Astrophysical Observatory # Ricardo Zanmar Sanchez INAF - OACT # Mariusz Gromadzki Warsaw Astronomical Observatory # Laurent Eyer University of Geneva 57497a64bb0ee362a07fe3846921fbc67cb03339 2334 2333 2018-09-14T10:57:53Z Gsawgwikiadmin 1 /* Registration is now open! */ wikitext text/x-wiki == <big>Registration is now close!</big> == <!-- <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> --> Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) if you would like to join the meeting at the very last minute! == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory # Giuseppe Leto INAF - Catania Astrophysical Observatory # Ricardo Zanmar Sanchez INAF - OACT # Mariusz Gromadzki Warsaw Astronomical Observatory # Laurent Eyer University of Geneva ee2017b406787de8091aef5296986921721d687d 2348 2334 2018-10-02T14:31:53Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now close!</big> == <!-- <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> --> Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) if you would like to join the meeting at the very last minute! == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory # Giuseppe Leto INAF - Catania Astrophysical Observatory # Ricardo Zanmar Sanchez INAF - OACT # Mariusz Gromadzki Warsaw Astronomical Observatory # Laurent Eyer University of Geneva # Peter Abraham Konkoly, Hungary # Gabor Marton Konkoly, Hungary ea842f1fe6417d302f7d5bafaf16ee3aefbfcd4d 2349 2348 2018-10-02T14:36:22Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now closed!</big> == <!-- <big>'''[https://goo.gl/forms/HeDrdgyL2QqBTpye2 REGISTRATION FORM]'''</big> --> Please email Lukasz Wyrzykowski (lw a t astrouw.edu.pl) if you would like to join the meeting at the very last minute! == Registered participants == # Meredith Morrell The Open University # Fraser Lewis Faulkes Telescope Project/National Schools' Observatory # Steve Boudreault Max Planck Institute for Solar System Research # Goran Damljanovic Astronomical Observatory # Ashish Mahabal Caltech # Suvi Gezari University of Maryland # Charlotte Ward University of Maryland # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław # Michel Dennefeld IAP/Sorbonne University # Marius Maskoliunas Vilnius University, Institute of Theoretical Physics and Astronomy # Erika Pakštienė Vilnius University, Institute of Theoretical Physics and Astronomy # Mihael Petac SISSA # Andreja Gomboc University of Nova Gorica # Anna Marciniak Adam Mickiewicz University # Tanja Petrushevska University of Nova Gorica # Katja Bricman University of Nova Gorica # Simon Hodgkin Institute of Astronomy, Cambridge University # Tonny Vanmunster Center for Backyard Astrophysics CBA # Franz-Josef Hambsch ROAD observatory # Pawel Zielinski Warsaw University Astronomical Observatory # Areg Mickaelian Byurakan Astrophysical Observatory (BAO) # Gor Mikayelyan Byurakan Astrophysical Observatory # Algita Stankevičiūtė Warsaw University Astronomical Observatory # Michał Pawlak Charles University in Prague # Katarzyna Kruszynska University of Warsaw, Faculty of Physics, Astronomical Observatory # Krzysztof Rybicki Warsaw University Astronomical Observatory # Lukasz Wyrzykowski Warsaw University Astronomical Observatory # Giuseppe Leto INAF - Catania Astrophysical Observatory # Ricardo Zanmar Sanchez INAF - OACT # Mariusz Gromadzki Warsaw Astronomical Observatory # Laurent Eyer University of Geneva # Peter Abraham Konkoly, Hungary # Gabor Marton Konkoly, Hungary 4e630aca35bc22fcd27bdc9d026cd98bb050abe8 6 304 2338 2018-09-22T15:59:06Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2342 2338 2018-09-24T16:23:48Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda-programme.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 303 2352 2351 2018-10-02T14:41:59Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |25 |---- |18:00 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Simon Hodgkin |Gaia Marshall |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- a1ee6c30806f31125f591589e4b81176ad985ecf 2358 2352 2018-10-04T11:00:01Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Simon Hodgkin |Gaia Marshall |25 |---- |18:00 |''end of day 1'' | | |---- |19:00 |wine tasting |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- 46da236e45a12329905142fc0b48e10fd8f966bf 2359 2358 2018-10-04T11:00:38Z Gsawgwikiadmin 1 /* Detailed programme */ wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Simon Hodgkin |Gaia Marshall |25 |---- |18:00 |''end of day 1'' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |'''Tuesday 9.10.2018''' | | | |---- |09:30 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |19:00 |'''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |'''Wednesday 10.10.2018''' | | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |trip to Postojna Cave | | |---- 4c8e732b2f12bcf14243ad97b9c9456b04e05087 2360 2359 2018-10-07T11:14:14Z Nada.ihanec 43 /* Detailed programme */ wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Draft agenda as PDF (subject to changes)]] '''Sunday 7th October 2018''' 19:00 Welcome drink at the University of Nova Gorica '''Monday 8th October 2018''' 09:30 bus leaves from Gold Club hotel 09:00 - 11:00 registration, coffee 11:00 start of the workshop evening: wine tasting (free) with optional dinner '''Tuesday 9th October 2018''' ''evening: workshop dinner'' '''Wednesday 10th October 2018''' ''12:30 lunch and end of the workshop'' optional trip to Postojna Cave == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Simon Hodgkin |Gaia Marshall |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- 2c79f630ee98bd2c7fc70fc45ef0320371e5b170 2361 2360 2018-10-09T15:33:21Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Agenda as PDF (subject to changes)]] == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |ZTF and Gaia synnergy for classification of sources |45 |---- |14:45 |Michał Pawlak |The ASAS-SN survey |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Simon Hodgkin |Gaia Marshall |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- 41fbc50c9ea44558bc2088fd1a6084e4a2a87721 2368 2361 2018-11-28T07:04:28Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Agenda as PDF (subject to changes)]] == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |Gaia Photometric Science Alerts: Status |45 |---- |12:00 |Laurent Eyer |GAIA Variables and plans for DR3 |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AshishMahabal.pdf ZTF and Gaia synergy for classification of sources] |45 |---- |14:45 |Michał Pawlak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MichalPawlak.pdf The ASAS-SN survey] |30 |---- |15:15 |Steve Boudreault |PLATO Science Flux Alerts |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |Asteroid studies supported by Gaia |30 |---- |16:40 |Lukasz Wyrzykowski |OPTICON network for time-domain astronomy |25 |---- |17:05 |Pawel Zielinski |Cambridge Photometric Calibration Server 2.0 |30 |---- |17:35 |Simon Hodgkin |Gaia Marshall |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |Young Stellar Objects in Gaia and improvements of the detection algorithms |30 |---- |10:00 |Lukasz Wyrzykowski |Black holes with microlensing |30 |---- |10:30 |Katarzyna Kruszynska |Photometric Gravitational Microlensing observed by Gaia |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |Astrometric microlensing with Gaia |20 |---- |11:50 |Zofia Kaczmarek |Lensing by intermediate-mass black holes in Gaia |15 |---- |12:05 |Algita Stankevičiūtė |Astrometry with VLTI and GRAVITY |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |Lensed supernovae: the past and the future |20 |---- |14:20 |Areg Mickaelian |Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs |20 |---- |14:40 |Valeria Grisoni |Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era |15 |---- |14:55 |Mihael Petac |The importance of Gaia mission for Dark Matter searches |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |Energetic extragalactic transients |20 |---- |16:00 |Katja Bricman |TDEs with LSST |15 |---- |16:15 |Mariusz Gromadzki |Highlights from Warsaw hunt for TDEs |20 |---- |16:35 |Nada Ihanec |Gaia and OGLE TDE search |20 |---- |16:55 |Fraser Lewis |Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research |15 |---- |17:10 |Meredith Morrell |The Open University Contribution to Gaia Alerts Photometric Follow Up |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert) |25 |---- |09:55 |Tonny Vanmunster |Pro-Am Photometric Projects with Robotic Observatories |25 |---- |10:20 |Przemysław Mikołajczyk |Status of the Bialkow observatory |20 |---- |10:40 |Giuseppe Leto |INAF OACT facility in Sicily |15 |---- |10:55 |'''coffee break''' | |30 |---- |11:25 |Michel Dennefeld |Results from OHP |15 |---- |11:40 |Goran Damljanovic |Serbian-Bulgarian activities in line with Gaia Alerts during 2018 |15 |---- |11:55 |Marius Maskoliunas |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- 17da7adb8875144ee734ea2744c31653f49ee62d 2369 2368 2018-11-28T07:13:25Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Agenda as PDF (subject to changes)]] == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin1.pdf Gaia Photometric Science Alerts: Status] |45 |---- |12:00 |Laurent Eyer |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LaurentEyer.pdf Gaia Variables and plans for DR3] |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AshishMahabal.pdf ZTF and Gaia synergy for classification of sources] |45 |---- |14:45 |Michał Pawlak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MichalPawlak.pdf The ASAS-SN survey] |30 |---- |15:15 |Steve Boudreault |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SteveBoudreault.pdf PLATO Science Flux Alerts] |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AnnaMarciniak.pdf Asteroid studies supported by Gaia] |30 |---- |16:40 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski1.pdf OPTICON network for time-domain astronomy] |25 |---- |17:05 |Pawel Zielinski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PawelZielinski.pdf Cambridge Photometric Calibration Server 2.0] |30 |---- |17:35 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin2.pdf Gaia Marshall] |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GaborMarton.pdf Young Stellar Objects in Gaia and improvements of the detection algorithms] |30 |---- |10:00 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski2.pdf Black holes with microlensing] |30 |---- |10:30 |Katarzyna Kruszynska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatarzynaKruszynska.pdf Photometric Gravitational Microlensing observed by Gaia] |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KrisRybicki.pdf Astrometric microlensing with Gaia] |20 |---- |11:50 |Zofia Kaczmarek |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ZofiaKaczmarek.pdf Lensing by intermediate-mass black holes in Gaia] |15 |---- |12:05 |Algita Stankevičiūtė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AlgitaStankeviciute.pdf Astrometry with VLTI and GRAVITY] |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TanjaPetrushevska.pdf Lensed supernovae: the past and the future] |20 |---- |14:20 |Areg Mickaelian |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AregMickaelian.pdf Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs] |20 |---- |14:40 |Valeria Grisoni |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ValeriaGrisoni.pdf Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era] |15 |---- |14:55 |Mihael Petac |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MihaelPetac.pdf The importance of Gaia mission for Dark Matter searches] |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AndrejaGomboc.pdf Energetic extragalactic transients] |20 |---- |16:00 |Katja Bricman |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatjaBricman.pdf TDEs with LSST] |15 |---- |16:15 |Mariusz Gromadzki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariuszGromadzki.pdf Highlights from Warsaw hunt for TDEs] |20 |---- |16:35 |Nada Ihanec |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/NadaIhanec.pdf Gaia and OGLE TDE search] |20 |---- |16:55 |Fraser Lewis |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/FraserLewis.pdf Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research] |15 |---- |17:10 |Meredith Morrell |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MeredithMorrell.pdf The Open University Contribution to Gaia Alerts Photometric Follow Up] |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/JoschHambsch.pdf Highlights from 7 years on the ROAD (Remote Observatory Atacama] Desert) |25 |---- |09:55 |Tonny Vanmunster |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TonnyVanmunster.pdf Pro-Am Photometric Projects with Robotic Observatories] |25 |---- |10:20 |Przemysław Mikołajczyk |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PrzemekMikolajczyk.pdf Status of the Bialkow observatory] |20 |---- |10:40 |Giuseppe Leto |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GiuseppeLeto.pdf INAF OACT facility in Sicily] |15 |---- |10:55 |'''coffee break''' | |40 |---- |11:40 |Goran Damljanovic |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GoranDamljanovic.pdf Serbian-Bulgarian activities in line with Gaia Alerts during 2018] |15 |---- |11:55 |Marius Maskoliunas |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:05 |Erika Pakštienė |Moletai Astronomical Observatory in context of Gaia alerts |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- 81de375a06064f715e6ecc17d62acad9244c102b 2370 2369 2018-11-28T07:14:24Z Gsawgwikiadmin 1 /* Detailed programme */ wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Agenda as PDF (subject to changes)]] == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin1.pdf Gaia Photometric Science Alerts: Status] |45 |---- |12:00 |Laurent Eyer |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LaurentEyer.pdf Gaia Variables and plans for DR3] |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AshishMahabal.pdf ZTF and Gaia synergy for classification of sources] |45 |---- |14:45 |Michał Pawlak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MichalPawlak.pdf The ASAS-SN survey] |30 |---- |15:15 |Steve Boudreault |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SteveBoudreault.pdf PLATO Science Flux Alerts] |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AnnaMarciniak.pdf Asteroid studies supported by Gaia] |30 |---- |16:40 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski1.pdf OPTICON network for time-domain astronomy] |25 |---- |17:05 |Pawel Zielinski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PawelZielinski.pdf Cambridge Photometric Calibration Server 2.0] |30 |---- |17:35 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin2.pdf Gaia Marshall] |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GaborMarton.pdf Young Stellar Objects in Gaia and improvements of the detection algorithms] |30 |---- |10:00 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski2.pdf Black holes with microlensing] |30 |---- |10:30 |Katarzyna Kruszynska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatarzynaKruszynska.pdf Photometric Gravitational Microlensing observed by Gaia] |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KrisRybicki.pdf Astrometric microlensing with Gaia] |20 |---- |11:50 |Zofia Kaczmarek |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ZofiaKaczmarek.pdf Lensing by intermediate-mass black holes in Gaia] |15 |---- |12:05 |Algita Stankevičiūtė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AlgitaStankeviciute.pdf Astrometry with VLTI and GRAVITY] |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TanjaPetrushevska.pdf Lensed supernovae: the past and the future] |20 |---- |14:20 |Areg Mickaelian |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AregMickaelian.pdf Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs] |20 |---- |14:40 |Valeria Grisoni |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ValeriaGrisoni.pdf Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era] |15 |---- |14:55 |Mihael Petac |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MihaelPetac.pdf The importance of Gaia mission for Dark Matter searches] |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AndrejaGomboc.pdf Energetic extragalactic transients] |20 |---- |16:00 |Katja Bricman |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatjaBricman.pdf TDEs with LSST] |15 |---- |16:15 |Mariusz Gromadzki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariuszGromadzki.pdf Highlights from Warsaw hunt for TDEs] |20 |---- |16:35 |Nada Ihanec |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/NadaIhanec.pdf Gaia and OGLE TDE search] |20 |---- |16:55 |Fraser Lewis |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/FraserLewis.pdf Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research] |15 |---- |17:10 |Meredith Morrell |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MeredithMorrell.pdf The Open University Contribution to Gaia Alerts Photometric Follow Up] |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/JoschHambsch.pdf Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert)] |25 |---- |09:55 |Tonny Vanmunster |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TonnyVanmunster.pdf Pro-Am Photometric Projects with Robotic Observatories] |25 |---- |10:20 |Przemysław Mikołajczyk |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PrzemekMikolajczyk.pdf Status of the Bialkow observatory] |20 |---- |10:40 |Giuseppe Leto |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GiuseppeLeto.pdf INAF OACT facility in Sicily] |15 |---- |10:55 |'''coffee break''' | |40 |---- |11:40 |Goran Damljanovic |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GoranDamljanovic.pdf Serbian-Bulgarian activities in line with Gaia Alerts during 2018] |15 |---- |11:55 |Marius Maskoliunas |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:05 |Erika Pakštienė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- bb3d78b46b96adb4415067cc94658ba2414306c2 2371 2370 2018-12-03T07:58:51Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Agenda as PDF (subject to changes)]] == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin1.pdf Gaia Photometric Science Alerts: Status] |45 |---- |12:00 |Laurent Eyer |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LaurentEyer.pdf Gaia Variables and plans for DR3] |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AshishMahabal.pdf ZTF and Gaia synergy for classification of sources] |45 |---- |14:45 |Michał Pawlak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MichalPawlak.pdf The ASAS-SN survey] |30 |---- |15:15 |Steve Boudreault |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SteveBoudreault.pdf PLATO Science Flux Alerts] |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AniaMarciniak.pdf Asteroid studies supported by Gaia] |30 |---- |16:40 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski1.pdf OPTICON network for time-domain astronomy] |25 |---- |17:05 |Pawel Zielinski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PawelZielinski.pdf Cambridge Photometric Calibration Server 2.0] |30 |---- |17:35 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin2.pdf Gaia Marshall] |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GaborMarton.pdf Young Stellar Objects in Gaia and improvements of the detection algorithms] |30 |---- |10:00 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski2.pdf Black holes with microlensing] |30 |---- |10:30 |Katarzyna Kruszynska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatarzynaKruszynska.pdf Photometric Gravitational Microlensing observed by Gaia] |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KrisRybicki.pdf Astrometric microlensing with Gaia] |20 |---- |11:50 |Zofia Kaczmarek |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ZofiaKaczmarek.pdf Lensing by intermediate-mass black holes in Gaia] |15 |---- |12:05 |Algita Stankevičiūtė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AlgitaStankeviciute.pdf Astrometry with VLTI and GRAVITY] |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TanjaPetrushevska.pdf Lensed supernovae: the past and the future] |20 |---- |14:20 |Areg Mickaelian |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AregMickaelian.pdf Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs] |20 |---- |14:40 |Valeria Grisoni |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ValeriaGrisoni.pdf Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era] |15 |---- |14:55 |Mihael Petac |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MihaelPetac.pdf The importance of Gaia mission for Dark Matter searches] |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AndrejaGomboc.pdf Energetic extragalactic transients] |20 |---- |16:00 |Katja Bricman |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatjaBricman.pdf TDEs with LSST] |15 |---- |16:15 |Mariusz Gromadzki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariuszGromadzki.pdf Highlights from Warsaw hunt for TDEs] |20 |---- |16:35 |Nada Ihanec |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/NadaIhanec.pdf Gaia and OGLE TDE search] |20 |---- |16:55 |Fraser Lewis |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/FraserLewis.pdf Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research] |15 |---- |17:10 |Meredith Morrell |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MeredithMorrell.pdf The Open University Contribution to Gaia Alerts Photometric Follow Up] |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/JoschHambsch.pdf Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert)] |25 |---- |09:55 |Tonny Vanmunster |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TonnyVanmunster.pdf Pro-Am Photometric Projects with Robotic Observatories] |25 |---- |10:20 |Przemysław Mikołajczyk |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PrzemekMikolajczyk.pdf Status of the Bialkow observatory] |20 |---- |10:40 |Giuseppe Leto |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GiuseppeLeto.pdf INAF OACT facility in Sicily] |15 |---- |10:55 |'''coffee break''' | |40 |---- |11:40 |Goran Damljanovic |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GoranDamljanovic.pdf Serbian-Bulgarian activities in line with Gaia Alerts during 2018] |15 |---- |11:55 |Marius Maskoliunas |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:05 |Erika Pakštienė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |Workshop summary |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- ac9de92bc59ac3a6b28ac491412154ff071ccd66 2372 2371 2019-01-25T05:53:18Z Gsawgwikiadmin 1 /* Detailed programme */ wikitext text/x-wiki The programme will be composed of invited and contributed talks and will be prepared after the registration is closed. ---- [[Media:agenda-programme.pdf | Agenda as PDF (subject to changes)]] == Detailed programme == {| class="wikitable" | |'''name''' |'''title''' |'''time (with discussion)''' |---- |---- |'''Monday 8.10.2018''' | | | |---- |09:30 |'''bus to Vipava registration and coffee''' | | |---- |11:00 | |Welcome by the organizers |15 |---- |11:15 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin1.pdf Gaia Photometric Science Alerts: Status] |45 |---- |12:00 |Laurent Eyer |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LaurentEyer.pdf Gaia Variables and plans for DR3] |30 |---- |12:30 |'''lunch''' | |90 |---- |14:00 |Ashish Mahabal |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AshishMahabal.pdf ZTF and Gaia synergy for classification of sources] |45 |---- |14:45 |Michał Pawlak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MichalPawlak.pdf The ASAS-SN survey] |30 |---- |15:15 |Steve Boudreault |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SteveBoudreault.pdf PLATO Science Flux Alerts] |20 |---- |15:35 |'''coffee break''' | |35 |---- |16:10 |Anna Marciniak |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AniaMarciniak.pdf Asteroid studies supported by Gaia] |30 |---- |16:40 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski1.pdf OPTICON network for time-domain astronomy] |25 |---- |17:05 |Pawel Zielinski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PawelZielinski.pdf Cambridge Photometric Calibration Server 2.0] |30 |---- |17:35 |Simon Hodgkin |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/SimonHodgkin2.pdf Gaia Marshall] |25 |---- |18:00 |''end of day 1'' | | |---- |18:30 |'''bus transfer from Lanthieri mansion to wine-tasting''' | | |---- |19:00 |'''wine tasting''' |http://www.vinajamsek.si/ | |---- |cca 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Tuesday 9.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Gabor Marton, Peter Abraham |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GaborMarton.pdf Young Stellar Objects in Gaia and improvements of the detection algorithms] |30 |---- |10:00 |Lukasz Wyrzykowski |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/LukaszWyrzykowski2.pdf Black holes with microlensing] |30 |---- |10:30 |Katarzyna Kruszynska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatarzynaKruszynska.pdf Photometric Gravitational Microlensing observed by Gaia] |30 |---- |11:00 |'''coffee break''' | |30 |---- |11:30 |Krzysztof Rybicki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KrisRybicki.pdf Astrometric microlensing with Gaia] |20 |---- |11:50 |Zofia Kaczmarek |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ZofiaKaczmarek.pdf Lensing by intermediate-mass black holes in Gaia] |15 |---- |12:05 |Algita Stankevičiūtė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AlgitaStankeviciute.pdf Astrometry with VLTI and GRAVITY] |15 |---- |12:20 |'''lunch break''' | |100 |---- |14:00 |Tanja Petrushevska |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TanjaPetrushevska.pdf Lensed supernovae: the past and the future] |20 |---- |14:20 |Areg Mickaelian |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AregMickaelian.pdf Gaia DR2 and statistical analysis of the Catalogue of White Dwarfs] |20 |---- |14:40 |Valeria Grisoni |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/ValeriaGrisoni.pdf Chemical evolution models for the Milky Way thick and thin discs in the Gaia Era] |15 |---- |14:55 |Mihael Petac |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MihaelPetac.pdf The importance of Gaia mission for Dark Matter searches] |15 |---- |15:10 |'''coffee break''' | |30 |---- |15:40 |Andreja Gomboc |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/AndrejaGomboc.pdf Energetic extragalactic transients] |20 |---- |16:00 |Katja Bricman |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/KatjaBricman.pdf TDEs with LSST] |15 |---- |16:15 |Mariusz Gromadzki |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariuszGromadzki.pdf Highlights from Warsaw hunt for TDEs] |20 |---- |16:35 |Nada Ihanec |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/NadaIhanec.pdf Gaia and OGLE TDE search] |20 |---- |16:55 |Fraser Lewis |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/FraserLewis.pdf Using Gaia Alerts and the Faulkes Telescope to Bridge Between Education and Research] |15 |---- |17:10 |Meredith Morrell |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MeredithMorrell.pdf The Open University Contribution to Gaia Alerts Photometric Follow Up] |15 |---- |17:25 |''end of day 2'' | | |---- |18:30 |bus transfer to '''workshop dinner''' |https://gostilna-theodosius.si/ | |---- |cca. 21:30 |'''bus transfer back to Ajdovščina''' | | |---- |'''Wednesday 10.10.2018''' | | | |---- |9:00 |'''bus transfer from Gold Club Hotel in Ajdovščina to Lanthieri mansion''' | | |---- |09:30 |Franz-Josef Hambsch |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/JoschHambsch.pdf Highlights from 7 years on the ROAD (Remote Observatory Atacama Desert)] |25 |---- |09:55 |Tonny Vanmunster |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/TonnyVanmunster.pdf Pro-Am Photometric Projects with Robotic Observatories] |25 |---- |10:20 |Przemysław Mikołajczyk |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/PrzemekMikolajczyk.pdf Status of the Bialkow observatory] |20 |---- |10:40 |Giuseppe Leto |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GiuseppeLeto.pdf INAF OACT facility in Sicily] |15 |---- |10:55 |'''coffee break''' | |40 |---- |11:40 |Goran Damljanovic |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/GoranDamljanovic.pdf Serbian-Bulgarian activities in line with Gaia Alerts during 2018] |15 |---- |11:55 |Marius Maskoliunas |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:05 |Erika Pakštienė |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/MariusMaskoliunas.pdf Moletai Astronomical Observatory in context of Gaia alerts] |10 |---- |12:15 |Lukasz Wyrzykowski & Andreja Gomboc |[http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2018/slides/WorkshopSummary.pdf Workshop summary] |15 |---- |12:30 |''end of day 3'' | | |---- |12:30 |'''lunch''' | | |---- |14:00 |'''bus transfer from Lanthieri mansion to Postojna Cave''' | | |---- |cca. 17:00-18:00 |'''bus transfer from Postojna Cave to Ajdovščina''' | | |---- c93a35d23fa46f7dbfb14a29516ce19135e98bfb 6 304 2353 2342 2018-10-02T14:44:00Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda-programme.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2357 2353 2018-10-04T10:59:34Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda-programme.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 200 2354 2209 2018-10-04T08:39:11Z Gsawgwikiadmin 1 wikitext text/x-wiki The main address of the server is: http://gsaweb.ast.cam.ac.uk/followup == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. Updated December 2016 by LW. == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org = Data Policy = If you use any of the data from the Calibration Server in your publication, please acknowledge it with the following text: '''We acknowledge the use of the Cambridge Photometric Calibration Server (http://gsaweb.ast.cam.ac.uk/followup), developed and maintained by Lukasz Wyrzykowski and Sergey Koposov, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890 (OPTICON).''' If the data is essential for the paper, please include the observers as co-authors. 666d852be14703ec58535424cc02bb67e2980809 2355 2354 2018-10-04T09:19:46Z Gsawgwikiadmin 1 /* Data Policy */ wikitext text/x-wiki The main address of the server is: http://gsaweb.ast.cam.ac.uk/followup == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. Updated December 2016 by LW. == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org = Data Policy = If you use any of the data from the Calibration Server in your publication, please acknowledge it with the following text: ''' We acknowledge the use of the Cambridge Photometric Calibration Server (http://gsaweb.ast.cam.ac.uk/followup), developed and maintained by Lukasz Wyrzykowski, Sergey Koposov, Arancha Delgado, Pawel Zielinski, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890 (OPTICON). ''' If the data is essential for the paper, please include the observers as co-authors. bcc3ffff60460d76838c2abebe704b953901af3c 2356 2355 2018-10-04T09:20:00Z Gsawgwikiadmin 1 /* Data Policy */ wikitext text/x-wiki The main address of the server is: http://gsaweb.ast.cam.ac.uk/followup == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. Updated December 2016 by LW. == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org = Data Policy = If you use any of the data from the Calibration Server in your publication, please acknowledge it with the following text: '''We acknowledge the use of the Cambridge Photometric Calibration Server (http://gsaweb.ast.cam.ac.uk/followup), developed and maintained by Lukasz Wyrzykowski, Sergey Koposov, Arancha Delgado, Pawel Zielinski, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890 (OPTICON).''' If the data is essential for the paper, please include the observers as co-authors. 295f61c2c3252242805a7c09d34edc93d9b173de 0 293 2362 2294 2018-10-09T15:34:55Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights * machine-learning classification of transients * Gaia Alerts and DR2 * new photometric calibration server * organization of the follow-up ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) === Workshop Photo === [[File:workshop2018Vipava.jpg|left|450px|photo2018]] dad269456b1af259876f4cc0504e6a7ad7144883 2364 2362 2018-10-09T15:39:07Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights * machine-learning classification of transients * Gaia Alerts and DR2 * new photometric calibration server * organization of the follow-up ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) === Workshop Photo === [[File:workshop2018Vipava_small.jpg|left|450px|photo2018]] c83212b730e2f1005d2f856433d02f1a952bc516 2366 2364 2018-10-09T15:54:36Z Gsawgwikiadmin 1 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights * machine-learning classification of transients * Gaia Alerts and DR2 * new photometric calibration server * organization of the follow-up ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) === Workshop Photo === [[File:workshop2018Vipava_small.jpg | workshop2018Vipava.jpg|left|450px|photo2018]] 6eecac91fde50f7f1f8f9de2bb5e9e7c47a588e5 2367 2366 2018-10-09T15:55:36Z Gsawgwikiadmin 1 /* Workshop Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2018-small.png|right|450px|poster2018]] '''The ninth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2018:logistics | Vipava/Slovenia, 8 - 10 Oct. 2018]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights * machine-learning classification of transients * Gaia Alerts and DR2 * new photometric calibration server * organization of the follow-up ---- * [[workshop2018:rationale|Rationale]] * [[workshop2018:agenda|Agenda]] * [[workshop2018:registration|Registration]] * [[workshop2018:logistics|Logistic information]] * [[workshop2018:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Andreja Gomboc (Nova Gorica) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Nova Gorica) * Tanja Petrushevska (Nova Gorica) * Katja Bricman (Nova Gorica) * Aurora Clerici (Nova Gorica) === Workshop Photo === [[File:workshop2018Vipava.jpg|left|450px|photo2018]] dad269456b1af259876f4cc0504e6a7ad7144883 6 305 2363 2018-10-09T15:36:30Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 306 2365 2018-10-09T15:39:30Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 1 2373 2284 2019-03-29T06:37:52Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania, Sicily, 18-20 December 2019]]</Big>''' </center> ---- <center> [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 0cc266e2736ef63a67cea60171ddd2b96664cb4b 0 307 2374 2019-03-29T06:40:48Z Gsawgwikiadmin 1 Created page with "== Welcome! == <!---[[File:Poster2019-small.png|right|450px|poster2019]] ---> '''The tenth OPTICON Gaia Science Alerts workshop will be held in Workshop2019:logistics | Cat..." wikitext text/x-wiki == Welcome! == <!---[[File:Poster2019-small.png|right|450px|poster2019]] ---> '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * new members of the network * new photometric calibration server * organization of the follow-up * future plans ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) 8aa0cb9cf33f3fb0731c9b8fffb2eb6a9f3024f5 2383 2374 2019-09-10T13:08:21Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!---[[File:Poster2019-small.png|right|450px|poster2019]] ---> '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy transient surveys * new members of the telescope network * new photometric calibration server * organization of the follow-up * future plans ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) 3ca6fbc010f981c2d7b6fca9452a322764a496fa 2384 2383 2019-09-13T05:24:05Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == <!---[[File:Poster2019-small.png|right|450px|poster2019]] ---> '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy transient surveys * new members of the telescope network * new photometric calibration server * organization of the follow-up * future plans ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) 673b040bc8c85267e320dd0e5a748aea41bdaf43 2385 2384 2019-09-13T05:24:59Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == <!---[[File:Poster2019-small.png|right|450px|poster2019]] ---> '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) 3e96ecb8d607be5d93fffafc68d6c4df6ab535b0 2399 2385 2019-09-26T01:39:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) 8bc594c51a3af6c1f9264762672ccad22f3c96f6 8 3 2375 2287 2019-03-29T06:47:39Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2019 **workshop2019:main|Main Workshop Page **workshop2019:rationale|Rationale **workshop2019:agenda|Program **workshop2019:registration|Participants and Registration **workshop2019:logistics|Logistics *workshop 2018 **workshop2018:main|Main Workshop Page **workshop2018:agenda|Archive of presentations *workshop 2017 **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 1cedad1c4354dbcc54f5e5273abb4a2b19101ef8 0 308 2376 2019-04-23T06:34:06Z Gsawgwikiadmin 1 Created page with "Registration will open in June 2019. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl." wikitext text/x-wiki Registration will open in June 2019. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. 6d095b58abe744d865f90eca20bbd3d6cbce43f8 2377 2376 2019-04-23T06:34:58Z Gsawgwikiadmin 1 wikitext text/x-wiki Registration will open in June 2019 and will close Nov 1st. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. 7d5399c217d9fafb4def947cd9565a6626e9f250 2378 2377 2019-08-04T11:26:18Z Gsawgwikiadmin 1 wikitext text/x-wiki Registration will open in late August 2019 and will close Nov 1st. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. 5a4916841812dc3a7ae360a729181e51f5333089 2379 2378 2019-08-04T11:26:31Z Gsawgwikiadmin 1 wikitext text/x-wiki Registration will open in late August 2019 and will close Nov 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. c426c00aef2589f427bd8f775ccab3245f2c56eb 2380 2379 2019-08-29T14:29:29Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 REGISTRATION FORM]'''</big> The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. 996487048feba17f9f539cacea46867cb95233a4 2392 2380 2019-09-25T21:36:54Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 REGISTRATION FORM]'''</big> The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. === Note: there is no registration fee thanks to the generous support of the OPTICON grant === ae51234521d4f113ba4b4d07b5a7722727df5faf 2393 2392 2019-09-25T21:37:09Z Gsawgwikiadmin 1 wikitext text/x-wiki == <big>Registration is now open!</big> == <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 REGISTRATION FORM]'''</big> The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. = Note: there is no registration fee thanks to the generous support of the OPTICON grant = 1ba72f072760dd1ac14b747bc4b40bc830620e33 2394 2393 2019-09-25T21:37:22Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 REGISTRATION FORM]'''</big> The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl. ==== Note: there is no registration fee thanks to the generous support of the OPTICON grant ==== fcfae1b1aace6d62914a8bec46800aceaa0aecc7 2395 2394 2019-09-25T21:37:36Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl ==== ==== Note: there is no registration fee thanks to the generous support of the OPTICON grant ==== 3d98112baf6a2733d799325ff333ee8374f1f66a 2396 2395 2019-09-25T21:37:53Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl ==== ==== Note: there is no registration fee thanks to the generous support of the OPTICON grant ==== d6cb4fce7b99f756265cfaf56b9381b7c97d4112 2397 2396 2019-09-25T21:38:13Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl ==== Note: there is no registration fee thanks to the generous support of the OPTICON grant. 9713406d0fdf295f9be7431e0d08fb5d6c4d0908 2398 2397 2019-09-25T21:38:24Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl Note: there is no registration fee thanks to the generous support of the OPTICON grant. 5c5b479e24ef2f5a91976dac8903b96a30a16a2f 0 309 2381 2019-08-30T13:44:08Z Gsawgwikiadmin 1 Created page with "We plan to start in the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. You could also reserve the Saturday for a potential social event, bu..." wikitext text/x-wiki We plan to start in the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. You could also reserve the Saturday for a potential social event, but the details will be confirmed soon. 18526f62cc9164b926b89f1fd0151bf3fee8a78e 2382 2381 2019-08-30T13:44:17Z Gsawgwikiadmin 1 wikitext text/x-wiki We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. You could also reserve the Saturday for a potential social event, but the details will be confirmed soon. 9af2d8286549b3facc032cf1e658a1c56a6c13a9 0 310 2386 2019-09-13T05:29:43Z Gsawgwikiadmin 1 Created page with "= Workshop Venue = Catania Astrophysical Observatory / INAF- Osservatorio Astrofisico di Catania Via S.Sofia 78, 95123 Catania, ITALY = Travel Information = == By Air..." wikitext text/x-wiki = Workshop Venue = Catania Astrophysical Observatory / INAF- Osservatorio Astrofisico di Catania Via S.Sofia 78, 95123 Catania, ITALY = Travel Information = == By Air == == By Train == == By Bus == = Accommodation = = Social Program = 149c91d321360d1ec6d001ad273b471b1d800f09 2401 2386 2019-09-26T14:14:07Z Flavia.calderone 44 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = Catania Astrophysical Observatory / INAF- Osservatorio Astrofisico di Catania Via S.Sofia 78, 95123 Catania, ITALY Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. = Travel Information = == By Air == == By Train == == By Bus == = Accommodation = = Social Program = 9260b777a33c1e0be910da6a4983318f3e37237f 2402 2401 2019-09-26T14:28:06Z Flavia.calderone 44 /* By Air */ wikitext text/x-wiki = Workshop Venue = Catania Astrophysical Observatory / INAF- Osservatorio Astrofisico di Catania Via S.Sofia 78, 95123 Catania, ITALY Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. = Travel Information = == By Air == Here there are information about the main airports of the area and the distance by car/bus from the city center. '''CATANIA FONTANAROSSA AIRPORT''' | +15min The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl= Position on Google Maps] | [http://www.aeroporto.catania.it/= Airport Website] '''COMISO AIRPORT''' | +1h 40min Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7= Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/= Airport Website] == By Train == == By Bus == = Accommodation = = Social Program = 999fe28d3c69f5fa63eab46de0848b54fe5d3827 2403 2402 2019-09-26T15:11:34Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = Catania Astrophysical Observatory / INAF- Osservatorio Astrofisico di Catania <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. = Travel Information = The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. Here follows a wide overview of the possible ways to travel to Catania. == By Air == Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] == By Train == Catania Central Station is situated 1.4 km from the main squares of Catania. [https://www.trenitalia.com/it.html Trenitalia] offers connections from other cities in Italy and European countries. LINKS: [https://goo.gl/maps/ZvXNRTdsLSNYAcTP9 Position on Google Maps of the Central Railway Station] == By Bus == Bus service companies, such as https://www.eurolines.de/ Eurolines], [http://www.saistrasporti.it/= Sais Autolinee] and [https://shop.flixbus.it/ Flixbus], offers routes from other Italian cities and European countries to Catania. They usually stop at the Terminal Bus, near the Central Railway Station. Companies such as [http://www.astsicilia.it/ AST] and [http://www.amt.ct.it/ AMT] offer services for local transfers. LINKS: [https://goo.gl/maps/Jo46WBbfkSmnxfe4A= Position on Google Maps of the Terminal Bus] == By Ferry == Catania can be also reached by ferry from Salerno, Naples and Malta. It is also possible to arrive in other Sicilian ports, such as Messina, Milazzo and Palermo, and then move to Catania. LINKS: [https://www.traghettilines.it/ Traghettilines] | [https://www.grimaldi-lines.com/ Grimaldi Lines] | [http://www.virtuferries.com/ Virtu Ferries] | [https://www.adspmaresiciliaorientale.it/porto-di-catania/ Position on Google Maps of the Port] | [https://www.adspmaresiciliaorientale.it/porto-di-catania/ Port website] = Accommodation = = Social Program = dac373f32d4697d8679c6fb72ee92d11c0d36139 0 311 2387 2019-09-25T21:31:33Z Gsawgwikiadmin 1 Created page with "[[File:Poster2019-small.png|450px|poster2019]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG..." wikitext text/x-wiki [[File:Poster2019-small.png|450px|poster2019]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2019.png | here]] * Poster as a PDF [[Media:GaiaScienceAlertsWorkshopPoster2019.pdf | here]] bed52f1739b29e08c5a818466969ab844b52e855 6 313 2390 2019-09-25T21:33:51Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 314 2391 2019-09-25T21:36:13Z Gsawgwikiadmin 1 Created page with "Gaia is now a well established and leading transient mission. It discovers nearly 2000 objects a year from all over the sky, down to about 20 mag, covering all possible classe..." wikitext text/x-wiki Gaia is now a well established and leading transient mission. It discovers nearly 2000 objects a year from all over the sky, down to about 20 mag, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. The transient discovery machine within Gaia is constantly evolving and year 2019 brings many significant improvements and changes in the Gaia Alerts system and its operation. The long baseline of Gaia data allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such like flares in distant quasars, young stellar object, Be-type stars or microlensing events due to massive lenses. On the other hand, the evolution of the follow-up observations is also visible. Robotisation of telescope and queue-scheduled modes of operation of many telescopes allows for more efficient coordination for long-term time-domain astrophysical observations. The 2019 Gaia Alerts Workshop, the 10th in the series, will again be an opportunity to learn about Gaia and Gaia Alerts, to meet people behind the pipelines and web pages, to find out about most recent scientific highlights from Gaia Alerts and to discuss the scientific potential of this programme. 76f070b573ec0b3d7cd9975d0efd3a6c11ec0259 6 315 2400 2019-09-26T01:40:05Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 310 2404 2403 2019-09-26T16:17:07Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The 10th OPTICON Gaia Science Alerts Workshop will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. '''INAF - Astrophysical Observatory of Catania | INAF- Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. Here follows a wide overview of the possible ways to travel to Catania. == By Airplane == Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] == By Train == Catania Central Station is situated 1.4 km from the main squares of Catania. [https://www.trenitalia.com/it.html Trenitalia] offers connections from other cities in Italy and European countries. LINKS: [https://goo.gl/maps/ZvXNRTdsLSNYAcTP9 Position on Google Maps of the Central Railway Station] == By Bus == Bus service companies, such as https://www.eurolines.de/ Eurolines], [http://www.saistrasporti.it/= Sais Autolinee] and [https://shop.flixbus.it/ Flixbus], offers routes from other Italian cities and European countries to Catania. They usually stop at the Terminal Bus, near the Central Railway Station. Companies such as [http://www.astsicilia.it/ AST] and [http://www.amt.ct.it/ AMT] offer services for local transfers. LINKS: [https://goo.gl/maps/Jo46WBbfkSmnxfe4A= Position on Google Maps of the Terminal Bus] == By Ferry == Catania can be also reached by ferry from Salerno, Naples and Malta. It is also possible to arrive in other Sicilian ports, such as Messina, Milazzo and Palermo, and then move to Catania. LINKS: [https://www.traghettilines.it/ Traghettilines] | [https://www.grimaldi-lines.com/ Grimaldi Lines] | [http://www.virtuferries.com/ Virtu Ferries] | [https://www.adspmaresiciliaorientale.it/porto-di-catania/ Position on Google Maps of the Port] | [https://www.adspmaresiciliaorientale.it/porto-di-catania/ Port website] = Accommodation = = Social Program = de7f46c9574c6061d3901922e1546f929b6a7c3e 2406 2404 2019-10-04T08:23:35Z Flavia.calderone 44 /* Workshop Venue */ wikitext text/x-wiki = Workshop Venue = The 10th OPTICON Gaia Science Alerts Workshop will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. Here follows a wide overview of the possible ways to travel to Catania. == By Airplane == Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] == By Train == Catania Central Station is situated 1.4 km from the main squares of Catania. [https://www.trenitalia.com/it.html Trenitalia] offers connections from other cities in Italy and European countries. LINKS: [https://goo.gl/maps/ZvXNRTdsLSNYAcTP9 Position on Google Maps of the Central Railway Station] == By Bus == Bus service companies, such as https://www.eurolines.de/ Eurolines], [http://www.saistrasporti.it/= Sais Autolinee] and [https://shop.flixbus.it/ Flixbus], offers routes from other Italian cities and European countries to Catania. They usually stop at the Terminal Bus, near the Central Railway Station. Companies such as [http://www.astsicilia.it/ AST] and [http://www.amt.ct.it/ AMT] offer services for local transfers. LINKS: [https://goo.gl/maps/Jo46WBbfkSmnxfe4A= Position on Google Maps of the Terminal Bus] == By Ferry == Catania can be also reached by ferry from Salerno, Naples and Malta. It is also possible to arrive in other Sicilian ports, such as Messina, Milazzo and Palermo, and then move to Catania. LINKS: [https://www.traghettilines.it/ Traghettilines] | [https://www.grimaldi-lines.com/ Grimaldi Lines] | [http://www.virtuferries.com/ Virtu Ferries] | [https://www.adspmaresiciliaorientale.it/porto-di-catania/ Position on Google Maps of the Port] | [https://www.adspmaresiciliaorientale.it/porto-di-catania/ Port website] = Accommodation = = Social Program = 7276490c719a41290bd6ca3998c5c8f5b81ee980 2411 2406 2019-10-04T12:06:56Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The 10th OPTICON Gaia Science Alerts Workshop will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. Here follows a wide overview of the possible ways to travel to Catania. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania by Train, by Bus and by Ferry, please see [ here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one: here you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. For more information about the route of metro and shuttles, see the [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg map] (in red: the metro route; in yellow: shuttle route). <br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] = Accommodation = = Social Program = e839c96f6acdd1074840906d10022dd3a76d827f 2412 2411 2019-10-04T12:11:41Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. Here follows a wide overview of the possible ways to travel to Catania. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania by Train, by Bus and by Ferry, please see [ here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one: here you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. For more information about the route of metro and shuttles, see the [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg map] (in red: the metro route; in yellow: shuttle route). <br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] = Accommodation = = Social Program = 273383db66efc54b3fd0df061115457237d810a9 2413 2412 2019-10-04T12:13:05Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. Here follows a wide overview of the possible ways to travel to Catania. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [ here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one: here you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. For more information about the route of metro and shuttles, see the [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg map] (in red: the metro route; in yellow: shuttle route). <br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] = Accommodation = = Social Program = 181a3894ae84e96982ad405b6e05d9db79252c0c 2414 2413 2019-10-04T12:13:59Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [ here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one: here you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. For more information about the route of metro and shuttles, see the [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg map] (in red: the metro route; in yellow: shuttle route). <br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] = Accommodation = = Social Program = 4f5ecaf30fbc36df803adb6c2966a6ab956612bf 2415 2414 2019-10-04T12:22:31Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [ here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one: here you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] = Accommodation = = Social Program = 3a9dfde8a3dbfe0dbefa13d6894f28fb5fc5e5c7 2416 2415 2019-10-04T14:47:43Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm= Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels that are close to Bus or Metro stops. = Social Program = a847947c2366ce57a1fd34b58d2666442ca8be90 2417 2416 2019-10-04T14:49:47Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For other information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels that are close to Bus or Metro stops. = Social Program = f106eb46608dfe7bdb5148db55b1929b91937812 2419 2417 2019-10-04T15:14:04Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. Several airlines offer flights to many national and international destinations. From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus. From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels that are close to Bus or Metro stops. = Social Program = dc96f25ca65f5cd117f5e9caf91f6ddd92a7e554 2422 2419 2019-10-04T15:48:26Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach to Catania== The best way to reach Catania is by plane and public transport. Otherwise, other means of transport could be a good option too. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels that are close to Bus or Metro stops. = Social Program = 7a6617134d3c9fbfed84f53013105164f5bca15d 2426 2422 2019-10-05T08:02:10Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels that are close to Bus or Metro stops. = Social Program = 8a32633b4fd7fd1820655dc27fb6d83a2ad7306c 2427 2426 2019-10-05T08:03:35Z Flavia.calderone 44 /* Accommodation */ wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops. = Social Program = 209260435e54acd8ddd0819e7dbf8ff7f8ca8f63 2428 2427 2019-10-05T08:03:56Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops. = Social Program = d2f5dad2a16cee419eab28a49f0646f83f00ed4f 2435 2428 2019-10-18T07:45:24Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' = Social Program = 99df202b548f7f54dab881a98ef685af3fd11aa9 0 309 2405 2382 2019-10-03T20:20:07Z Gsawgwikiadmin 1 wikitext text/x-wiki We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! 7c9b6d897f311309a732bf70960165942e060bfe 2432 2405 2019-10-11T19:35:36Z Flavia.calderone 44 wikitext text/x-wiki We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! =Social dinner= The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> More information and details will follow soon.<br /> Please let us know if you are willing to attend the social dinner and indicate if you have any food intolerances or special requests. <br /> =Social event: excursion to Mount Etna= We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' Full details about the organization will be given later, but an approximate itinerary of the excursion may be: *leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *a guided tour of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); *lunch in the Sapienza Refuge area; *in the early afternoon, a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano at Serra La Nave (1.735 m asl); *return back to Catania about at 5:00 p.m. Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up with an organized tour that includes cab+unimog+guided tour: the fare is around €65. ==Fares for excursion to Mount Etna== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC. </br> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. ==What you need to know before joining the excursion== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] =Alternative trip to Syracuse= In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; *the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; *the ''Ortigia Island'' and the ''Duomo Cathedral''. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ==Fares for excursion to Syracuse== Transportation by bus from/to Catania is offered by the Meeting WOC. </br> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. badb0e4bd4bbeeb52239ff3e90d93963f02e6d45 2433 2432 2019-10-11T19:37:31Z Flavia.calderone 44 wikitext text/x-wiki We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! =Social dinner= The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> More information and details will follow soon.<br /> Please let us know if you are willing to attend the social dinner and indicate if you have any food intolerances or special requests. <br /> =Social event: excursion to Mount Etna= We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' Full details about the organization will be given later, but an approximate itinerary of the excursion may be: *leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *a guided tour of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); *lunch in the Sapienza Refuge area; *in the early afternoon, a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano at Serra La Nave (1.735 m asl); *return back to Catania about at 5:00 p.m. Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up with an organized tour that includes cab+unimog+guided tour: the fare is around €65. ==Fares for excursion to Mount Etna== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. ==What you need to know before joining the excursion== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] =Alternative trip to Syracuse= In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; *the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; *the ''Ortigia Island'' and the ''Duomo Cathedral''. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ==Fares for excursion to Syracuse== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. f8a1bdbde0230299d0dee372093e97935db84b92 0 307 2407 2399 2019-10-04T11:08:56Z Flavia.calderone 44 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) 392a86d5bbb6f7498bc0a9ef2987234a6c806aae 6 316 2408 2019-10-04T11:41:24Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2409 2408 2019-10-04T11:44:17Z Flavia.calderone 44 Flavia.calderone uploaded a new version of [[File:OsservatorioOACT.jpg]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 317 2410 2019-10-04T11:55:23Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 318 2418 2019-10-04T15:02:34Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 319 2420 2019-10-04T15:23:56Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 320 2421 2019-10-04T15:28:34Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 308 2423 2398 2019-10-04T16:57:17Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl Note: there is no registration fee thanks to the generous support of the OPTICON grant. === Preliminary list of participants (to be updated ) === # Przemysław Mikołajczyk # Mariusz Gromadzki # Fraser Lewis # Vytautas Cepas # Franz-Josef (Josch) Hambsch #Cosimo Inserra # Iair Arcavi # Goran Damljanovic # Tolga Güver # Gerry Gilmore # Susanne M Hoffmann # Vira Godunova # Krzysztof Hełminiak # Staszek Zola # Pawel Zielinski f554ab0eeda49fdd10c4267cbb9850c73cbc4aeb 2424 2423 2019-10-04T16:58:26Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of participants (to be updated ) === # Przemysław Mikołajczyk # Mariusz Gromadzki # Fraser Lewis # Vytautas Cepas # Franz-Josef (Josch) Hambsch #Cosimo Inserra # Iair Arcavi # Goran Damljanovic # Tolga Güver # Gerry Gilmore # Susanne M Hoffmann # Vira Godunova # Krzysztof Hełminiak # Staszek Zola # Pawel Zielinski d79480bc91a23450cd6521fc9abb8bd049f9d9d4 2425 2424 2019-10-04T17:00:17Z Gsawgwikiadmin 1 /* Preliminary list of participants (to be updated ) */ wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk # Mariusz Gromadzki # Fraser Lewis # Vytautas Cepas # Franz-Josef (Josch) Hambsch #Cosimo Inserra # Iair Arcavi # Goran Damljanovic # Tolga Güver # Gerry Gilmore # Susanne M Hoffmann # Vira Godunova # Krzysztof Hełminiak # Staszek Zola # Pawel Zielinski 11bd411b8f958d9c90b0ce69247b2d4ea4432abf 2434 2425 2019-10-16T20:38:06Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk # Mariusz Gromadzki # Fraser Lewis # Vytautas Cepas # Franz-Josef (Josch) Hambsch #Cosimo Inserra # Iair Arcavi # Goran Damljanovic # Tolga Güver # Gerry Gilmore # Susanne M Hoffmann # Vira Godunova # Krzysztof Hełminiak # Staszek Zola # Pawel Zielinski # Yana Markus # John Davies aa954490387e0430c8818c4d0ad94d750e44bcb8 2436 2434 2019-10-22T10:43:41Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Non 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) e6ec047c53770f6ca9258e0516a2d8d9c2820e5c 2437 2436 2019-10-23T20:38:59Z Gsawgwikiadmin 1 /* Registration is now open! */ wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) c89f0d57439865eedb63d5a3d38153d380d39219 2438 2437 2019-10-23T20:40:29Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) 78795474e2b337d42d111caa35fe52df6f69a293 2439 2438 2019-10-26T17:10:27Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) 07c231ea95a1a7cc2c831aa1d63e479a1242b9c9 2447 2439 2019-11-09T01:22:53Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) 149e516ca76db88acd18ebea41b7f5a9c939067a 2448 2447 2019-11-11T04:05:49Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) 6861fa1971ce6e73f6fd9b2c1f1b2b66729305c2 2449 2448 2019-11-11T04:40:21Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Cardiff University, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) cc890cd6c55a66c162efbbaac1e88857135927b2 2450 2449 2019-11-11T04:41:04Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) f7a8fcfd7a146b8443c70ba2848026c127a2e095 2451 2450 2019-11-11T04:41:35Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) c1515c2fee9ece5cfb3de3cc58096ee5b86c5190 2452 2451 2019-11-13T07:02:45Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) d52dccbe399731bae6499fd08b8e6bca357e44f2 2453 2452 2019-11-13T21:20:57Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) 00b0a02a16611c052b43d544928478188d2e4304 2454 2453 2019-11-14T18:11:51Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) b571ed87f7578c7bfd317a76be2bdddde1528ee4 2455 2454 2019-11-16T05:32:06Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> ==== The registration will close Nov 15th. ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) 3f6defa71d8a92b3ede840e65c7a3d93ddea6568 6 321 2429 2019-10-11T18:29:05Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 322 2430 2019-10-11T18:57:22Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 323 2431 2019-10-11T19:19:03Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 324 2442 2019-11-03T20:46:20Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 311 2443 2387 2019-11-03T20:47:02Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster2019-small.png|450px|poster2019]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[File:poster2019.png | here]] * Poster as a PDF [[File:GaiaScienceAlertsWorkshopPoster2019.pdf | here]] 07bf62ae1c7253925a6501bc680d4e981a02681d 2446 2443 2019-11-03T20:49:11Z Gsawgwikiadmin 1 wikitext text/x-wiki [[File:Poster2019-small.png|450px|poster2019]] ---- '''Feel free to download the workshop poster to spread the information about it in your institution''' * Poster as a PNG [[Media:poster2019.png | here]] * Poster as a PDF [[Media:GaiaScienceAlertsWorkshopPoster2019.pdf | here]] bed52f1739b29e08c5a818466969ab844b52e855 6 313 2444 2390 2019-11-03T20:47:44Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2019.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 315 2445 2400 2019-11-03T20:48:41Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:GaiaScienceAlertsWorkshopPoster2019.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 308 2456 2455 2019-11-16T05:33:51Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) 3450a1ab04ac33edb44e60ae9eeb819e441e70e6 2457 2456 2019-11-16T05:34:06Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Yana Pichkurova University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) 03360fab8caf1d15ea4278c048be4ebad901b0e0 2459 2457 2019-11-19T07:11:53Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Stephen M. Brincat (Flarestar Observatory, Malta) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) 533e8711542d2ef1f3a92de4bcd1da64522af868 2465 2459 2019-11-22T04:25:33Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) #David Buckley (South African Observatory) d731a7f47b558fa12fa0251c46ec95da412cea8e 2466 2465 2019-11-25T06:26:49Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Krzysztof Hełminiak (University of Toruń, Poland) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) #David Buckley (South African Astronomical Observatory) dbe1a45642c002b7ce228c8f8eb3999cb0ec67f8 2468 2466 2019-12-02T03:48:04Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) #David Buckley (South African Astronomical Observatory) da2a9c42a9a16194ab294fabf159ed459f25f272 2469 2468 2019-12-02T20:23:59Z Flavia.calderone 44 /* Preliminary list of registered participants (to be updated) */ wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) #David Buckley (South African Astronomical Observatory) #Sergio Messina (INAF Catania, Italy) e824f1ecfa5f7e366f1ba57160e63388542dc42c 2470 2469 2019-12-04T07:45:57Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- = <big>Registration is now open!</big> = --> <!-- <big>'''[https://forms.gle/SRDUA2KFpz24yf1J9 CLICK HERE FOR THE REGISTRATION FORM]'''</big> --> ==== The registration is now closed ==== In case of any enquires please email Lukasz Wyrzykowski lw at astrouw.edu.pl <span style="color:#009000"> Note: there is no registration fee thanks to the generous support of the OPTICON grant. </span> === Preliminary list of registered participants (to be updated) === # Przemysław Mikołajczyk (University of Wrocław, Poland) # Mariusz Gromadzki (University of Warsaw, Poland) # Fraser Lewis (Faulkes Telescope Project/National Schools Observatory, UK) # Vytautas Cepas (University of Vilnius, Lithuania) # Franz-Josef (Josch) Hambsch (ROAD Observatory Chile, Belgium) #Cosimo Inserra (Cardiff University, UK) # Iair Arcavi (Tel Aviv University, Israel) # Goran Damljanovic (Belgrade Observatory, Serbia) # Tolga Güver (Istanbul University, Turkey) # Gerry Gilmore (University of Cambridge, UK) # Susanne Hoffmann (Jena, Germany) # Vira Godunova (University of Kiyv, Ukraine) # Staszek Zola (Jagiellonian University, Krakow, Poland) # Pawel Zielinski (University of Warsaw, Poland) # Gábor Marton (Konkoly Observatory, Hungary) # Yana Markus (University of Kiyv, Ukraine) # John Davies (Royal Observatory Edinburgh) # Inna Izviekova (University of Kiyv, Ukraine) # Nada Ihanec (University of Warsaw, Poland) # Lorenzo Rimoldini (University of Geneva, Switzerland) # Ilknur Gezer (University of Warsaw, Poland) # Helen Jermak (Liverpool University, UK) # Jun Yang (MIT, USA) #Giuseppe Leto (INAF, Catania, Italy) #Krzysztof Rybicki (University of Warsaw, Poland) #Andrii Simon (University of Kiyv, Ukraine) #Volodymyr Reshetnyk (University of Kiyv, Ukraine) #Erika Pakstiene (University of Vilnius, Lithuania) #Mitja Fridman (University of Nova Gorica, Slovenia) # Oliwia Ziółkowska (University of Warsaw, Poland) # Gudrun Pebody (University of Cambridge, UK) # Katarzyna Kruszyńska (University of Warsaw, Poland) # Kotryna Siskauskaite (University of Vilnius, Lithuania) # Ricardo Zanmar Sanchez (INAF Catania, Italy) # Łukasz Wyrzykowski (University of Warsaw, Poland) #Flavia Calderone (INAF Catania, Italy) #Algita Stankevičiūtė (University of Warsaw, Poland) #Katja Bricman (University of Nova Gorica, Slovenia) #Marco Lam (Liverpool Telescope, UK) #Akihiko Fukui (University of Tokyo, Japan) #Marcin Gawroński (Nicolaus Copernicus University, Toruń, Poland) #Alisa Shchurova (Astronomical Institute Slovak Academy of Sciences, Slovakia) #Nariman Ismailov (Astrophysical Observatory, National Academy of Sciences, Azerbaijan) #Timo Prusti (ESA, NL) #Justas Zdanavičius (University of Vilnius, Lithuania) #Isabella Pagano (INAF Catania, Italy) #Mateusz Bronikowski (University of Warsaw, Poland) #Maria Isabel Carnerero Martin (INAF-Osservatorio Astrofisico di Torino, Italy) #Massimo Villata (INAF, Osservatorio Astrofisico di Torino, Italy) #Claudia M. Raiteri (INAF-Osservatorio Astrofisico di Torino, Italy) #Agnieszka Gurgul (Warsaw University Astronomical Observatory, Poland) #David Buckley (South African Astronomical Observatory) #Sergio Messina (INAF Catania, Italy) #Zofia Kaczmarek (University of Warsaw, Poland) e0aa747f2f424cf28c7617cba7bbf01539185fc6 0 309 2458 2433 2019-11-16T05:36:31Z Gsawgwikiadmin 1 /* Fares for excursion to Mount Etna */ wikitext text/x-wiki We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! =Social dinner= The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> More information and details will follow soon.<br /> Please let us know if you are willing to attend the social dinner and indicate if you have any food intolerances or special requests. <br /> =Social event: excursion to Mount Etna= We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' Full details about the organization will be given later, but an approximate itinerary of the excursion may be: *leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *a guided tour of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); *lunch in the Sapienza Refuge area; *in the early afternoon, a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano at Serra La Nave (1.735 m asl); *return back to Catania about at 5:00 p.m. Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up with an organized tour that includes cab+unimog+guided tour: the fare is around €65. ==Fares for excursion to Mount Etna== <!-- Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> --> The price of the trip will depend on the number of interested people. The price will include the transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area. All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. ==What you need to know before joining the excursion== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] =Alternative trip to Syracuse= In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; *the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; *the ''Ortigia Island'' and the ''Duomo Cathedral''. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ==Fares for excursion to Syracuse== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 9f3f2d4c5178e3ca4211a1ee7ce8cbb6d04f40d6 2460 2458 2019-11-19T07:15:20Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= It will appear here soon! We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! =Social dinner= The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> More information and details will follow soon.<br /> Please let us know if you are willing to attend the social dinner and indicate if you have any food intolerances or special requests. <br /> =Social event: excursion to Mount Etna= We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' Full details about the organization will be given later, but an approximate itinerary of the excursion may be: *leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *a guided tour of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); *lunch in the Sapienza Refuge area; *in the early afternoon, a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano at Serra La Nave (1.735 m asl); *return back to Catania about at 5:00 p.m. Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up with an organized tour that includes cab+unimog+guided tour: the fare is around €65. ==Fares for excursion to Mount Etna== <!-- Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> --> The price of the trip will depend on the number of interested people. The price will include the transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area. All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. ==What you need to know before joining the excursion== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] =Alternative trip to Syracuse= In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; *the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; *the ''Ortigia Island'' and the ''Duomo Cathedral''. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ==Fares for excursion to Syracuse== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. a8e8f3c269f4640fefe040c3109de7f01d3ffd77 2461 2460 2019-11-19T07:18:48Z Gsawgwikiadmin 1 Replaced content with "=Workshop Agenda= It will appear here soon! We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner..." wikitext text/x-wiki =Workshop Agenda= It will appear here soon! We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! cf52f7aec35c09f3988057692145fe8021b05f2f 2463 2461 2019-11-19T07:20:07Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= It will appear here soon! We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Logistics pages|Workshop2019:logistics]] 1bb646387b2fdac8b171d8a5d156792adb4abe33 2464 2463 2019-11-19T07:20:20Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= It will appear here soon! We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 441e1b79ce0fe2361d9ea9a087b20599028de06c 2471 2464 2019-12-07T03:51:38Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[Media:agenda.pdf PDF here]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 0f0dc810615ee043401f6efdb3097d0de15254bd 2472 2471 2019-12-07T03:51:48Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[Media:agenda.pdf|PDF here]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 0ae2cc8356d9df65fc11b136128e9c7d64ca8466 2474 2472 2019-12-07T03:52:37Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[File:agenda.pdf|PDF here]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] fb2a8c6dd8c8e75c0f721dc29844b8a6adf445f5 2475 2474 2019-12-07T03:52:52Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[File:agenda.pdf PDF here]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 808bc50a4920845fa80f9c883dc4a74baed72091 2476 2475 2019-12-07T03:53:05Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [File:agenda.pdf PDF here] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] f9da0b07a51a10d141793450431506060e1aa3a5 2477 2476 2019-12-07T03:53:17Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[File:agenda.pdf| PDF here]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 519024586919cd87cb090a30c73daad809b0b1a3 2478 2477 2019-12-07T03:53:32Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[PDF here|File:agenda.pdf]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 35fc2ba02de8ccd93ab161cc7b8716ce3c5ca715 2479 2478 2019-12-07T03:53:54Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= Draft agenda available as a [[Media:agenda.pdf|PDF here]] We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 0ae2cc8356d9df65fc11b136128e9c7d64ca8466 2480 2479 2019-12-07T03:54:19Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <big>Draft agenda available as a [[Media:agenda.pdf|PDF here]]</big> We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 26f48b0f9f3ba3c9072598c5f3c600fd6bf93af0 2481 2480 2019-12-07T03:54:30Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Draft agenda available as a [[Media:agenda.pdf|PDF here]]</Big> We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 88d0e7336cd20292a83e3054abb81a3dc711ba28 2482 2481 2019-12-07T03:54:44Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Draft agenda available as a [[Media:agenda.pdf|PDF here]]</Big> ---- We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 5fd691703d8bc74c80748f295c5872fdc2907262 2490 2482 2019-12-12T00:33:40Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Draft agenda available as a [[File:agenda.pdf|PDF here]]</Big> ---- We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] e8a7faeea3d05f1406b25a56d39f9e7c7e6b674f 2492 2490 2019-12-12T00:34:25Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Draft agenda available as a [[Media:agenda.pdf|PDF here]]</Big> ---- We plan to start on the morning of Wednesday, 18.Dec and finish the meeting with lunch on Friday, 20.Dec. The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 5fd691703d8bc74c80748f295c5872fdc2907262 0 310 2462 2435 2019-11-19T07:19:05Z Gsawgwikiadmin 1 /* Social Program */ wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social dinner= The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> More information and details will follow soon.<br /> =Social event: excursion to Mount Etna= We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' Full details about the organization will be given later, but an approximate itinerary of the excursion may be: *leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *a guided tour of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); *lunch in the Sapienza Refuge area; *in the early afternoon, a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano at Serra La Nave (1.735 m asl); *return back to Catania about at 5:00 p.m. Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up with an organized tour that includes cab+unimog+guided tour: the fare is around €65. ==Fares for excursion to Mount Etna== <!-- Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> --> The price of the trip will depend on the number of interested people. The price will include the transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area. All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. ==What you need to know before joining the excursion== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] =Alternative trip to Syracuse= In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; *the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; *the ''Ortigia Island'' and the ''Duomo Cathedral''. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ==Fares for excursion to Syracuse== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 3bb5fdaebcd66fc02af561d818163081621f3a5a 2467 2462 2019-11-27T13:15:12Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Aula Ovest” (West Hall), located on the ground floor of the Astrophysical Observatory. [[File:OsservatorioOACT.jpg|800px]] '''INAF - Astrophysical Observatory of Catania | INAF - Osservatorio Astrofisico di Catania''' <br /> Via S.Sofia 78, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach the INAF Astrophysical Observatory of Catania from the city center== INAF Astrophysical Observatory of Catania is close to downtown but up on a hill inside the “Policlinico Gaspare Rodolico” General Hospital area and near the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/yRUF8s5J3NfExugs7 Position on Google Maps] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] From city center you can reach the venue by public transport, such as Metro and BRT1 Bus.From the entrance of Policlinico, which address is Via S. Sofia n.78, the Observatory gathers for a 8-minute walk. <br />However, if you prefer to use taxi, you can tell the driver to leave you inside the Observatory parking area. [[File:Obspath1.png|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the Observatory is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Policlinico” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the Hospital area (“Policlinico” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the Observatory. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 at Vineria Picasso, in the city center of Catania.<br /> Click [https://goo.gl/maps/jGN9rbUx6Lbwuhwr5 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. f558725a550c693bfd7200a4c6cacf0c34f9df87 2488 2467 2019-12-12T00:20:28Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Light Blue Hall), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach INFN from the city center== The National Institute for Nuclear Physics is close to downtown but in the “Cittadella” University campus of Catania. The Workshop will held in the LNS Department, with is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [[File:INFN_Inquadramento.jpeg|800px]] From city center you can reach the venue by public transport, such as Metro Shuttle and BRT1 Bus. From the entrance of INFN, which address is Via S. Sofia n.62, the "Azzurra" room gathers for a 3-minute walk. <br /> See the following image to reach the room. [[File:INFN_Percorso2.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the INFN is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Cittadella Universitaria (Ovest)” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 9e2cfec884772f0437b31fcb526e4eb8659000a6 2495 2488 2019-12-12T00:41:00Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Light Blue Hall), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from Observatory rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach INFN from the city center== The National Institute for Nuclear Physics is close to downtown but in the “Cittadella” University campus of Catania. The Workshop will held in the '''LNS Department''', with is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [[File:INFN_Inquadramento.jpeg|800px]] From city center you can reach the venue by public transport, such as Metro Shuttle and BRT1 Bus. From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> See the following image to reach the room. [[File:INFN_Percorso3.jpg|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the INFN is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Cittadella Universitaria (Ovest)” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the Observatory to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. bd7c5b761c084a665deaf181b1b0a967ef557899 2496 2495 2019-12-12T00:43:39Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Light Blue Hall), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] ==How to reach INFN from the city center== The National Institute for Nuclear Physics is close to downtown but in the “Cittadella” University campus of Catania. The Workshop will held in the '''LNS Department''', with is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [[File:INFN_Inquadramento.jpeg|800px]] From city center you can reach the venue by public transport, such as Metro Shuttle and BRT1 Bus. From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> See the following image to reach the room. [[File:INFN_Percorso3.jpg|800px]] *'''By Metro + Metro Shuttle''' <br /> The closest metro stop to the INFN is the “Milo” one, from where you can reach the venue by a free Metro Shuttle service, stopping at the “Cittadella Universitaria (Ovest)” bus stop. <br />The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />The shuttles have frequency of a bus every 10 minutes.<br /> LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 86004045da003352311e408c5cc710daea666449 2497 2496 2019-12-12T11:37:54Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The '''National Institute for Nuclear Physics''' (INFN), located in Via S. Sofia n.62, is close to downtown but in the “Cittadella” University campus of Catania. <br /> The Workshop will held in the "Azzurra" Room at the '''LNS Department''', which is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research.<br /> LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. <br /> When you arrive to the INFN or leave the venue, for security reason please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). <br /> You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. <br />Buses are frequent: the shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] '''NOTICE''' At the entrance (point 2) you MUST tell your name at the Reception, they have the complete list of the participants and let you enter. When you leave the INFN please REMEMBER to go back to the Reception office (point 2) and get your daily presence unchecked. Returning to "Milo" Metro station: In the image that shows the bus path, the red line indicates the route of the shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. The bus end stop is at the "Milo" Metro Station that you will reach in 10 minutes. Buses are frequent. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 32ede8df690e71b73822453adeae3edb93d202a6 2498 2497 2019-12-12T11:41:48Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The '''National Institute for Nuclear Physics''' (INFN), located in Via S. Sofia n.62, is close to downtown but in the “Cittadella” University campus of Catania. <br /> The Workshop will held in the "Azzurra" Room at the '''LNS Department''', which is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research.<br /> LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. <br /> When you arrive to the INFN or leave the venue, for security reason please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] '''NOTICE''' At the entrance (point 2) you MUST tell your name at the Reception, they have the complete list of the participants and let you enter. When you leave the INFN please REMEMBER to go back to the Reception office (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 286e98868ed1bd7f7a3c3cebf4baf80d55baea45 2499 2498 2019-12-12T11:43:11Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The '''National Institute for Nuclear Physics''' (INFN), located in Via S. Sofia n.62, is close to downtown but in the “Cittadella” University campus of Catania. <br /> The Workshop will held in the "Azzurra" Room at the '''LNS Department''', which is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research.<br /> LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. <br /> When you arrive to the INFN or leave the venue, for security reason please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. c577b7f1ca18223794e2a97404a405983835de97 2500 2499 2019-12-12T11:44:23Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' will be held in Catania (Sicily - Italy) at the [http://home.infn.it/en/ National Institute for Nuclear Physics (INFN)] - [https://www.lns.infn.it/en/ LNS (Laboratori Nazionali del Sud) Department], with the collaboration of the INAF Astrophysical Observatory of Catania. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The '''National Institute for Nuclear Physics''' (INFN), located in Via S. Sofia n.62, is close to downtown but in the “Cittadella” University campus of Catania. <br /> The Workshop will held in the "Azzurra" Room at the '''LNS Department''', which is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research.<br /> LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reason please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 0a98f69b4ec1cc67793c467d1bfef8d22d1581ca 2501 2500 2019-12-12T11:52:40Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The '''National Institute for Nuclear Physics''' (INFN), located in Via S. Sofia n.62, is close to downtown but in the “Cittadella” University campus of Catania. <br /> The Workshop will held in the "Azzurra" Room at the '''LNS Department''', which is an important research center in the field of Nuclear Physics, Nuclear Astrophysics, Particle Astrophysics and Applied Research.<br /> LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reason please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. d83c28c99bacb7ab81c1d098958a3ab05d968379 2502 2501 2019-12-12T11:59:00Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The '''National Institute for Nuclear Physics''' (INFN), located in Via S. Sofia n.62, is close to downtown but in the “Cittadella” University campus of Catania. <br /> The Workshop will be held in the "Azzurra" Room at the '''LNS Department'''<br /> LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reason please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 06e9f1b27f417f6ecfff009ea1a247fc788d86ca 2503 2502 2019-12-12T12:03:07Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics''' (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. d7e8b16b113cc578f4f020625c47e610120603a8 2504 2503 2019-12-12T12:03:37Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicate the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 5e667c3b49cddc8dba3a1adaebe4f9251f9dc06b 2505 2504 2019-12-12T12:09:29Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the city center=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. edad2d34902c4c54367c204dc1ec5dbbaf636dcb 6 325 2473 2019-12-07T03:52:11Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2491 2473 2019-12-12T00:33:59Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2493 2491 2019-12-12T00:37:40Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 326 2483 2019-12-11T23:48:55Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 327 2484 2019-12-12T00:10:00Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 328 2485 2019-12-12T00:14:21Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2486 2485 2019-12-12T00:17:00Z Flavia.calderone 44 Flavia.calderone uploaded a new version of [[File:INFN Percorso2.jpeg]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2487 2486 2019-12-12T00:20:17Z Flavia.calderone 44 Flavia.calderone uploaded a new version of [[File:INFN Percorso2.jpeg]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2489 2487 2019-12-12T00:22:37Z Flavia.calderone 44 Flavia.calderone uploaded a new version of [[File:INFN Percorso2.jpeg]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 329 2494 2019-12-12T00:38:34Z Flavia.calderone 44 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 310 2506 2505 2019-12-12T13:06:52Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 89e7f7586575da130fdda973d0ac139b904e6973 2507 2506 2019-12-13T13:50:26Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here tell your name or show your badge and get your daily presence checked when you arrive and unchecked when you leave. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name at the Reception''', they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. ce132ecc07d4cacadff270e86f21a788af4bc8b5 2515 2507 2019-12-16T07:59:53Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 2f8082187bada0e8a3b7c0e1a54e32ef57bb44ef 2516 2515 2019-12-16T12:15:18Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' at 20:30 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 80fdd045f48b9b1ac5ed76c9d37ddfeb12fc517a 2526 2516 2019-12-19T08:57:44Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. e7cbc78a96eb486807ab0774280019c165206bf8 2528 2526 2019-12-19T11:16:28Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide on Friday afternoon. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. f7474f370ea554dd909a4baa9748339400d21f61 2537 2528 2019-12-19T15:10:28Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide on Friday afternoon. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. The appointment is at '''h 18.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. aaee856a6910948081af430aa5ad76c7df5a8a33 2538 2537 2019-12-19T15:10:49Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide on Friday afternoon. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. The appointment is at '''h 18.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. e081475cf9385a25ede72b9beecb310524832c10 2540 2538 2019-12-20T13:31:49Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> [https://goo.gl/maps/VxGsHnCbGmQjT1nt9 Position on Google Maps of "Piazza Stesicoro"] ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide on Friday afternoon. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. The appointment is at '''h 18.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 544a60413f33dad2c786743b49aae021a12b5916 2541 2540 2019-12-20T13:33:02Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide on Friday afternoon. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. The appointment is at '''h 18.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). [https://goo.gl/maps/VxGsHnCbGmQjT1nt9 Position on Google Maps of "Piazza Stesicoro"] ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' The appointment is at '''h 8.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). [https://goo.gl/maps/VxGsHnCbGmQjT1nt9 Position on Google Maps of "Piazza Stesicoro"] An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. 17f005dfd18a603f73899f097387a419dfc8ed84 2542 2541 2019-12-20T13:34:02Z Flavia.calderone 44 wikitext text/x-wiki = Workshop Venue = === <span style="color: red">Attention: change of building/room venue!</span> === The '''10th OPTICON Gaia Science Alerts Workshop''' is organized by INAF Astrophysical Observatory of Catania and is held in Catania (Sicily - Italy) at the '''National Institute for Nuclear Physics (INFN) - LNS (Laboratori Nazionali del Sud) Department'''. Workshop activities will take place in the “Sala Azzurra” (Azzurra Room), located on the first floor of the LSN Department. [[File:INFN_Catania.png|800px]] '''INFN - Laboratori Nazionali del Sud (LNS)''' <br /> Via S.Sofia 62, 95123 <br /> Catania, ITALY LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] | [http://home.infn.it/en/ INFN website] | [https://www.lns.infn.it/en/ LNS website] | [https://www.lns.infn.it/en/pratical-information/how-to-get-here.html How to reach LNS] | [http://www.oact.inaf.it/ INAF Astrophysical Observatory website] = Travel Information = [[File:main-palace-hotel-dintorni-catania-1.jpg|800px]] Catania is an ancient port city on the eastern coast of Sicily (Italy). <br />The city, located at the foot of volcano Etna, is noted for its history, culture, architecture and gastronomy and it is also a World Heritage Site, protected by UNESCO. [[File:etna-5.jpg|433px]] [[File:taormina1.jpg|363px]] LINKS: [https://goo.gl/maps/tEwTmDdobaXNGZNE9 Position on Google Maps] | [https://en.wikipedia.org/wiki/Catania Catania on Wikipedia] ==How to reach Catania== The best way to reach Catania is by plane. === By Airplane === Here there are information about the main airports of the area and the distance by car/bus from the city center. *'''CATANIA FONTANAROSSA AIRPORT''' | +15min <br /> The Fontanarossa International Airport is the closest airport to Catania. <br />Several airlines offer flights to many national and international destinations. <br />From Fontanarossa Airport is it possible to reach the City Center by Taxi or by Public transport. <br /> LINKS: [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl Position on Google Maps] | [http://www.aeroporto.catania.it/ Airport Website] *'''COMISO AIRPORT''' | +1h 40min <br /> Comiso Airport is a small airport located in Comiso (Ragusa), mainly connected by Ryanair flights. <br />From Comiso Airport there is a bus (Autolinee Giamporcaro) every few hours to get to Catania Central Station. <br />LINKS: [http://iltakkuino.altervista.org/inbus/autolineegiamporcaro/AeroportoCatania-AeroportoComiso-Vittoria.htm Bus timetable (Autolinee Giamporcaro)] | [https://goo.gl/maps/h72FV7Y9vqrJkvyX7 Position on Google Maps] | [http://www.aeroportodicomiso.eu/en/ Airport Website] For further information on how to reach Catania '''by Train''', '''by Bus''' and '''by Ferry''', please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing here]. ==How to reach Catania center from Fontanarossa Airport (and vice versa)== Catania Fontanarossa International Airport is the closest Airport to the city center. You can reach the downtown by taxi or bus. LINKS: [http://www.aeroporto.catania.it/?lang=en Airport Website] | [https://www.google.com/maps/place/Aeroporto+di+Catania-Fontanarossa/@37.4673046,15.0657746,15z/data=!4m5!3m4!1s0x0:0xec956aaf5d57793!8m2!3d37.4673046!4d15.0657746?shorturl=1 Position of the Fontanarossa Airport on Google Maps] | [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map] *'''BY TAXI (recommended)''' <br /> We recommend you to call [http://www.radiotaxicatania.org/it/ Radio-taxi] (+39 095 330966). <br />Call for a taxi (available h 24/24) when ready to leave the baggage claim area. The fare to the center is about €22, but you can ask for confirmation when you call. The airport to/from "Cittadella" University Campus rate is about €26. <br />Taxi picks you up in few minutes at the Airport on the Departure level (at the 1st floor): take the escalator or lift at your left after leaving the baggage claim area, then exit on the right and wait for your taxi. *'''BY PUBLIC TRANSPORT (ALIBUS)''' <br /> The [http://www.amt.ct.it/?page_id=2610 AMT Alibus Bus Service] leave every 25 minutes from 4:40 am to midnight, from the Airport to the City Center. <br />Bus ticket (€4) can be purchased: at the Airport; from authorized AMT retailers and AMT vending machines; on the bus; online with the UpMobile App. Remember to stamp the ticket upon getting on the bus. <br /> At the Fontanarossa Airport we suggest you use the bus stop located outside the Terminal A at the Arrival level (at ground floor, on your right after the exit), as reported on the [http://www.aeroporto.catania.it/files/image/Parcheggi/mappa-aeroporto_quadrata_1200x1200px.NEW.jpg Airport Parking Map]. <br />Please refer to the Alibus route and stops map to choose the bus stop closest to your Hotel.<br />LINKS: [http://www.amt.ct.it/blank.php?linea=ALIBUS&nome=Aeroporto,-,Centro&iframe=true&width=100%25&height=100%25 Alibus timetable – Price €4] | [http://www.amt.ct.it/wp-content/uploads/2016/08/Alibus4n.png Alibus route and stops] =How to reach the venue= The Workshop will be held at the "Azzurra" Room of the '''National Institute for Nuclear Physics (INFN) - LNS Department''', located in Via S. Sofia n.62, which is close to downtown but in the “Cittadella” University campus of Catania. LINKS: [https://goo.gl/maps/9dch8s74DSXNQ69G8 Position on Google Maps] ==From the the city center to INFN (and vice versa)== From city center you can reach the INFN by public transport, such as Metro Shuttle and BRT1 Bus. When you arrive to the INFN or leave the venue, for security reasons please '''REMEMBER to go to the Reception office''', which is located at the entrance in Via S. Sofia n.62: here '''tell your name or show the ID written on your badge''', so get your daily presence checked when you arrive and unchecked when you leave. The badge will speed-up operations. [[File:INFN_Inquadramento.jpeg|800px]] *'''By Metro + Metro Shuttle''' ''(recommended)'' <br /> The best way to reach Via Santa Sofia is by using the Metro. The closest metro stop to the INFN is the “Milo” Metro Station.<br />In the image the blue line indicates the Metro Shuttle path coming from "Milo" Metro Station to "Cittadella" University Campus, while the red line indicates the route of the Shuttle bus that returns back from Via Santa Sofia to the "Milo" Metro station. <br /> **<span style="color: blue>''From the "Milo" Metro Station to Via Santa Sofia''</span><br /> You can take the free Metro Shuttle Bus to University just outside Milo Station and then get out at the “Cittadella Universitaria (Ovest)” bus stop (the first one in Via S. Sofia). You do not need any extra ticket, because the metro ticket allows you to use the shuttle too.<br /> The metro trains have a frequency of one train every 10 minutes until 15:00; then the frequency will be one train every 15 minutes. The shuttles have frequency of a bus every 10 minutes. **<span style="color: red>''From Via Santa Sofia to the "Milo" Metro Station''</span><br /> If you want to reach the Metro Shuttle Bus Stop to come back to "Milo" Station, go to the entrance of INFN (Via S. Sofia n. 62) and then go towards the superior entrance (Via S. Sofia 64), enter and follow the road till the sign M-Bus (near the Math Department).<br />You do not need ticket to get on the Metro Shuttle, because the policy is that you will buy the metro ticket when you arrive to the "Milo" Metro Station. <br />LINKS: [https://www.circumetnea.it/upload/pdf%20orario%20analitico%20-%20metro%20Nesima%20%20Stesicoro.pdf Metro Timetable – Price €1,00 (90 minutes)] | [https://www.circumetnea.it/upload_news/ORARIO%20NAVETTA%20METRO%20SHUTTLE%20-%20In%20vigore%20dal%2019%20novembre%202018.pdf Metro Shuttle Timetable] | [https://universityequipe.com/wp-content/uploads/2017/09/shuttle-metro-catania.jpg Map of the Metro and Shuttles route (in red: the metro route; in yellow: shuttle route)] <br /> *'''BRT1 BUS''' <br /> The rapid bus [https://moovitapp.com/index/it/mezzi_pubblici-line-BRT1-Catania-2806-851990-268968-0 BRT1] connects downtown to the entrance of the University Campus area (“Cittadella Universitaria (Ovest)” bus stop). <br />Because BRT1 is a circular line, you can take this bus to go from the INFN to downtown at the same bus stop. <br />Buy a ticket also for the return trip. There are no places where to buy a ticket close to the venue. <br /> LINKS: [http://www.amt.ct.it/blank.php?linea=BRT1 BRT1 Timetable - €1.00 (90 minutes)] ===How to reach Sala Azzurra from the main entrance of the INFN=== From the entrance of INFN, which address is Via S. Sofia n.62, the '''"Azzurra" Room''' gathers for a 3-minute walk. <br /> The next image shows your way to reach the “Sala Azzurra” following the path from 1 to 10. [[File:INFN_Percorso3.jpg|800px]] ===='''NOTICE'''<br /> ==== At the entrance (point 2) you '''MUST tell your name and your ID (written on your Badge)''' at the Reception, because they have the complete list of the participants and let you enter. <br /> When you leave the INFN please '''REMEMBER to go back to the Reception office''' (point 2) and get your daily presence unchecked. For further information on logistics, please see [https://drive.google.com/file/d/1i7VWpCyg5e9vZBEX-JmkCIHbfpxhFtn1/view?usp=sharing this file] or contact our WOC staff at INAF Astrophysical Observatory of Catania: *Giuseppe Leto [mailto:giuseppe.leto@inaf.it] <br /> *Flavia Calderone [mailto:flavia.calderone@inaf.it] <br /> *Giancarlo Bellassai [mailto:giancarlo.bellassai@inaf.it] <br /> *Ricardo Zanmar Sanchez [mailto:ricardo.sanchez@inaf.it] <br /> = Accommodation = Here it is a [https://secure.booking.com/mywishlist.html?aid=304142&tflv=0&wl=ktruzcDmah1P%2FAYNPscsfnnhB7g& booking list] on www.booking.com of suggested city center hotels and B&B that are close to Bus or Metro stops.<br /> ''The Booking list offers the price for a double room by default: be careful to select the correct number of room guests before finalizing the reservation.'' =Social events= ==19.12.2019 | Social dinner== The Social Dinner will be held on '''Thursday 19th December''' h 20:00 at [https://materiaprimacatania.it Materia Prima], in the city center of Catania.<br /> Click [https://goo.gl/maps/N1GgFgsWPk6pm8nq6 here] for the position of the restaurant on Google Maps <br /> The dinner is fish-based, except for who are vegetarian and vegan, and it is offered by the Meeting WOC. <br /> ==20.12.2019 | Guided walking tour in the historical city center of Catania== We are planning to organize a private walking tour of the historic center of Catania with an english-speaking guide on Friday afternoon. Considering its status as an UNESCO World Heritage Site, Catania is full of history and ancient monuments and today boasts a rich cultural and architectural heritage to be discovered. <br /> The most remarkable landmarks are concentrated in the downtown area of Catania where, in addition to the Roman and Greek monuments, the streets are so attractive thanks to the magnificent Baroque architecture of the palaces, churches and monuments. The appointment is at '''h 18.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). <br /> [https://goo.gl/maps/VxGsHnCbGmQjT1nt9 Position on Google Maps of "Piazza Stesicoro"] ==21.12.2019 | Excursion to Mount Etna== We are are planning to organize an '''excursion on the Mount Etna''' for Saturday 21 December. <br /> For more information about Mount Etna, see the [https://en.wikipedia.org/wiki/Mount_Etna Wikipedia webpage]. [[File:etnacrateri3.jpg|373px]] [[File:Trekking-sullEtna-Cratere-Centrale--1080x675.jpg|424px]] <br /> ''Image credits: "Guide Vulcanologiche Etna" and "Rifugio Sapienza" websites'' The appointment is at '''h 8.00 in Piazza Stesicoro''' (by the side where you can find the ruins of the Roman amphitheater). <br /> [https://goo.gl/maps/VxGsHnCbGmQjT1nt9 Position on Google Maps of "Piazza Stesicoro"] An approximate itinerary of the excursion may be: *8:30 Leave Catania city center in the morning by bus to reach the Sapienza Refuge, which is located in the privileged position of 1.920 meters above sea level, at the highest point of arrival for cars and close to the Etna cable car facilities; *9:30 Arrival at the Sapienza Refuge *9:45 A guided tour (in English) of the area around Sapienza Refuge (within 200 m asl variation) or, for those who want to try a stronger experience, a trekking further up to 2.900 asl (depending on the Prefecture security prescriptions); for the fares of this second option, please see the section "Fares for excursion to Mount Etna" *13:00-14:30 Lunch in the Sapienza Refuge area; *15:00 Transfer by bus to Serra La Nave (1.735 m asl) for a visit to the station "M.G. Fracastoro" of the Catania Astrophysical Observatory, located on the southern slope of Mt. Etna volcano; *17:00 Return back to Catania about at 5:00 p.m.; *18:00 Arrival to Catania center. ===Fares for excursion to Mount Etna=== Transportation by bus from/to Catania and the guide for the tour around the Sapienza Refuge area are offered by the Meeting WOC.<br /> All meals, the trip on the higher craters and what is not explicitly indicated are the responsibility of the participants. <br /> Who wants to try a closer experience with craters in the morning can buy a ticket at Sapienza Refuge to go up to 2.900 asl with an organized tour that includes cab+unimog+guided tour: the fare is around €65. The price of the trip will depend on the number of interested people. <br /> ===What you need to know before joining the excursion=== *Mount Etna is the highest volcano in Europe (3.350 meters) and one of the most active volcanoes in the world. Following continuous eruptive activities, access beyond 2.920 meters asl ("Torre del Filosofo") is forbidden, as per the Ordinance of the Prefecture of Catania. *The mountain requires specific clothing and accessories: trekking shoes, anoraks and also walking stick are recommended (they can be rented at the Sapienza Refuge). We suggest you also to get dressed in layers, in order to cope with sudden climatic changes, and to bring with you some food and water. *This excursion is not recommended only for those who suffer from blood pressure, heart problems and asthma. LINKS: [https://www.rifugiosapienza.com/cosa-fare-sull-etna.php Rifugio Sapienza website] | [https://g.page/rifugio-sapienza?share Position of Sapienza Refuge on Google Maps] | [http://funiviaetna.com/ Funivia dell’Etna (Etna cable car)] | [https://en.wikipedia.org/wiki/Mount_Etna Mount Etna on Wikipedia] ==21.12.2019 | Alternative trip to Syracuse== In case of unfavorable weather conditions on the mountain, which in December could also foresee snow, an alternative could be a '''one-day trip to Syracuse'''.<br /> Syracuse, a historic sicilian city covered in layers of white stone, is listed since 2005 by UNESCO as a World Heritage Site because its monuments and archeological sites are charming example of different architectural and cultural historical periods, such as Greek, Roman and Baroque. [[File:1600px-Cattedrale,_Syracuse,_Province_of_Syracuse,_Ortygia,_Sicily,_Italy_-_panoramio.jpg|800px]] <br /> ''Image credits: "Wikimedia Commons" The trip itinerary is to be defined, but it may include: *8:30 Departure from Catania to Syracuse *10:00 Arrival to Syracuse and visit the Archaeological area with an English-speaking tourist guide; *13:00 Transfer by bus from Syracuse to Ortigia; lunch at Ortigia; *14:30 Guided tour (English spoken) of Ortigia, which may include: **''Neapolis archaeological park'', which is a vast area featuring many important ancient buildings and structures, such as Roman theater, Greek theater, the altar of Hieron II and the Ear of Dionysius; **the ''Syracuse market'', where you can shop souvenirs and even buy some spices and herbs; **the ''Ortigia Island'' and the ''Duomo Cathedral''; *17:00 Return back to Catania; *18:00 Arrival at Catania center. LINKS: [https://en.wikipedia.org/wiki/Syracuse,_Sicily Syracuse on Wikipedia] | [https://goo.gl/maps/EHQCy84t38y5qAnz7 Position of Syracuse on Google Maps] ===Fares for excursion to Syracuse=== Transportation by bus from/to Catania is offered by the Meeting WOC. <br /> All meals, tickets in the archeological sites and what is not explicitly indicated are the responsibility of the participants. fa9bb8170abee925dc4f5c1ed34b3a04fbf616fe 0 309 2508 2492 2019-12-13T19:26:46Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Draft agenda available as a [[Media:agenda.pdf|PDF here]]</Big> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' | |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 2f1fc8be44fa5657d67707fc8f685540388364b3 2509 2508 2019-12-13T19:33:34Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Agenda is available also as a [[Media:agenda.pdf|PDF here]]</Big> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' | |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |'''20:00''' | |'''Workshop Dinner''' | |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] aa687d4f740d9b508a218921a18bdcc80ce65253 2510 2509 2019-12-13T19:34:05Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Agenda is available also as a [[Media:agenda.pdf|PDF here]]</Big> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' | |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 8fe58c881d86e7d98a8ae320aa7a2c905d7a7aea 2511 2510 2019-12-13T19:34:29Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Agenda is available also as a [[Media:agenda.pdf|PDF here]]</Big> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' | |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 2660ec754c9a1b78f2724241bd69abfc2b9c52ab 2512 2511 2019-12-13T23:48:30Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' | |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] b000481081a82b3fff6d50b9c4c5d02459e7bcce 2513 2512 2019-12-13T23:48:42Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' | |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 1579933f2ac4c2f0720d6d3f523e62a6f2d8d041 2514 2513 2019-12-14T17:17:23Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |(remote) Gaia Science Alerts introduction |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 0e9399cb2db7dd1fcee80fb18b14d5aa32b1cd9f 2517 2514 2019-12-17T19:01:29Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] a72a75d7b03d603fb018bcf70fa3654360991d42 2518 2517 2019-12-17T19:01:50Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events |00:15 |---- |11:45 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:00 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:15 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:30 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:45 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:00 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:15''' |'''Lunch break ''' | |01:00 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 13/12/2019 11:05:31 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 5d11b94c61b69aef8fb4eeebdadaa35d4433408d 2519 2518 2019-12-17T19:03:56Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |17:45 |Jun Yang |Measure the gas to dust ratio towards bright sources in the Galactic Bulge |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] e8ecd862d2dc3fc300e5932b31fb9d6247a6cbde 2520 2519 2019-12-17T19:22:10Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> Agenda is available also as a [[Media:agenda.pdf|PDF here]] ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] a00aea9eec946933fc86cb6234413d6dfa6fd729 2521 2520 2019-12-17T19:22:36Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 7e5173db68cd7bdcadff9816397916c98db344d9 2522 2521 2019-12-18T11:53:51Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldinii.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 9f30c009479e5e0a42331a1afe5acfc821836c1f 2523 2522 2019-12-18T16:30:34Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldinii.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 6dc21fad53ad3ace8432790b27b682ce50c56a83 2524 2523 2019-12-18T16:31:32Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |Buckley David |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] aec45c3a72ea13e948911c3d70707ebc713b314d 2525 2524 2019-12-18T16:49:44Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON |00:15 |---- |10:20 |David Buckley |Transient astronomy in South Africa |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] f9f8e963f868637480564a6ca4ac119f40c80226 2527 2525 2019-12-19T10:42:31Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GerryGilmore.pdf PDF] |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GudrunPebody.pdf PDF] |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JohnDavies.pdf PDF] |00:15 |---- |10:20 |David Buckley |Transient astronomy in South Africa [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/DavidBuckley.pdf PDF] |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcoLam.pdf PDF] |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PawelZielinski.pdf PDF] |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PrzemekMikolajczyk.pdf PDF] |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LukaszWyrzykowski.pdf PDF] |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IairArcavi.pdf PDF] |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |12:50 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] f88d2273f3ad12748bd4cf4265ac4b33d275f5b8 2539 2527 2019-12-20T08:01:46Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GerryGilmore.pdf PDF] |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GudrunPebody.pdf PDF] |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JohnDavies.pdf PDF] |00:15 |---- |10:20 |David Buckley |Transient astronomy in South Africa [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/DavidBuckley.pdf PDF] |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcoLam.pdf PDF] |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PawelZielinski.pdf PDF] |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PrzemekMikolajczyk.pdf PDF] |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LukaszWyrzykowski.pdf PDF] |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IairArcavi.pdf PDF] |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes. |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON |00:15 |---- |12:35 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes |00:15 |---- |12:50 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory |00:15 |---- |13:05 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 17/12/2019 20:02 '' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 8f1140ba2b53b580bb9b295b5bf4089a4772eeba 2543 2539 2019-12-21T05:15:07Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GerryGilmore.pdf PDF] |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GudrunPebody.pdf PDF] |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JohnDavies.pdf PDF] |00:15 |---- |10:20 |David Buckley |Transient astronomy in South Africa [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/DavidBuckley.pdf PDF] |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcoLam.pdf PDF] |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PawelZielinski.pdf PDF] |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PrzemekMikolajczyk.pdf PDF] |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LukaszWyrzykowski.pdf PDF] |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IairArcavi.pdf PDF] |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RobBeswick.pdf PDF] |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcinGawronski.pdf PDF] |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/CosimoInserra.pdf PDF] |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MariuszGromadzki.pdf PDF] |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/NadaIhanec.pdf PDF] |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MateuszBronikowski.pdf PDF] |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KatjaBricman.pdf PDF] |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ZofiaKaczmarek.pdf PDF] |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AlgitaStankeviciute.pdf PDF] |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KotrynaSiskauskaite.pdf PDF] |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KatarzynaKruszynska.pdf PDF] |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KrzysztofRybicki.pdf PDF] |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AgnieszkaGurgul.pdf PDF] |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TolgaGuver.pdf PDF] |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/NarimanIsmailov.pdf PDF] |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/OliwiaZiolkowska.pdf PDF] |00:15 |---- |12:35 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/StaszekZola.pdf PDF] |00:15 |---- |12:50 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ErikaPakstiene.pdf PDF] |00:15 |---- |13:05 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JustasZdanavicius.pdf PDF] |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 21/12/2019 06:14'' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] 646623bdfe85c68a6a8cfff74b40f987188c59a1 2544 2543 2020-01-08T06:34:14Z Gsawgwikiadmin 1 wikitext text/x-wiki =Workshop Agenda= <!-- <Big>Zoom link to join the meeting streaming [https://zoom.us/j/456819731 https://zoom.us/j/456819731]</Big> --> <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GerryGilmore.pdf PDF] |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GudrunPebody.pdf PDF] |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JohnDavies.pdf PDF] |00:15 |---- |10:20 |David Buckley |Transient astronomy in South Africa [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/DavidBuckley.pdf PDF] |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcoLam.pdf PDF] |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PawelZielinski.pdf PDF] |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PrzemekMikolajczyk.pdf PDF] |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LukaszWyrzykowski.pdf PDF] |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IairArcavi.pdf PDF] |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RobBeswick.pdf PDF] |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcinGawronski.pdf PDF] |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/CosimoInserra.pdf PDF] |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MariuszGromadzki.pdf PDF] |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/NadaIhanec.pdf PDF] |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MateuszBronikowski.pdf PDF] |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KatjaBricman.pdf PDF] |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ZofiaKaczmarek.pdf PDF] |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AlgitaStankeviciute.pdf PDF] |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KotrynaSiskauskaite.pdf PDF] |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KatarzynaKruszynska.pdf PDF] |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KrzysztofRybicki.pdf PDF] |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AgnieszkaGurgul.pdf PDF] |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TolgaGuver.pdf PDF] |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/NarimanIsmailov.pdf PDF] |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/OliwiaZiolkowska.pdf PDF] |00:15 |---- |12:35 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/StaszekZola.pdf PDF] |00:15 |---- |12:50 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ErikaPakstiene.pdf PDF] |00:15 |---- |13:05 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JustasZdanavicius.pdf PDF] |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 21/12/2019 06:14'' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] d72de253aa798248c1af5ea0c8cff970e2d8a1c7 2551 2544 2020-06-17T06:09:24Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki =Workshop Agenda= <!--Agenda is available also as a [[Media:agenda.pdf|PDF here]] --> ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Wednesday 18 December 2019'''</big> |---- |'''10:00''' |'''Coffee and Registration ''' | |01:00 |---- |11:00 |Giuseppe Leto, Isabella Pagano | Welcome address and logistics |00:10 |---- |11:10 |Timo Prusti |Gaia mission status [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TimoPrusti.pdf PDF] |00:30 |---- |11:40 |Lorenzo Rimoldini |Classification of Gaia variable objects: DR2 vs DR3 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LorenzoRimoldini.pdf PDF] |00:20 |---- |12:00 |Simon Hodgkin |Gaia Science Alerts introduction (delivered by LW) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/SimonHodgkin.pdf PDF] |00:30 |---- |12:30 |Gábor Marton |PyTorch classification of astronomical light curves [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GaborMarton.pdf PDF] |00:15 |---- |12:45 |Mitja Fridman |Study of the Gaia AlertPipe performance and test of the likelihood detector [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MitjaFridman.pdf PDF] |00:15 |---- |'''13:00''' |'''Lunch break ''' | |01:00 |---- |14:00 |Akihiko Fukui |Planned Ground-based Survey for Bright Microlensing Events [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AkihikoFukui.pdf PDF] |00:25 |---- |14:25 |Ilknur Gezer |Young Stellar Objects in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IlknurGezer.pdf PDF] |00:15 |---- |14:40 |Volodymyr Reshetnyk |Gaia Alerts in X-ray and Radio catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/VolodymirReshetnyk.pdf PDF] |00:15 |---- |14:55 |Andrii Simon |New events in the Gaia alerts data. [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AndrewSimon.pdf PDF] |00:15 |---- |15:10 |Franz-Josef (Josch) Hambsch |Follow up of GAIA alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JoschHambsch.pdf PDF] |00:15 |---- |'''15:25''' |'''Coffee break''' | |00:35 |---- |16:00 |Fraser Lewis |(remote) Using Gaia Alerts to Link Education and Research [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/FraserLewis.pdf PDF] |00:15 |---- |16:15 |Vira Godunova |Long-term monitoring of Gaia transients at the Terskol Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ViraGodunova.pdf PDF] |00:15 |---- |16:30 |Inna Izviekova |Variability analysis of Gaia16bnz by optical follow-up from Terskol and Lisnyky observatories [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/InnaIzviekova.pdf PDF] |00:15 |---- |16:45 |Yana Markus |Gaia Alerts optical follow-up from Lisnyky observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/YanaMarkus.pdf PDF] |00:15 |---- |17:00 |Helen Jermak |Time Domain Astronomy with the New Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/HelenJermak.pdf PDF] |00:15 |---- |17:15 |Ricardo Zanmar Sanchez |News about the robotic APT2 telescope and the SOXS spectrograph at NTT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RicardoZanmarSanchez.pdf PDF] |00:15 |---- |17:30 |Susanne M Hoffmann |2000 years of alert history - what can we learn from dead astronomer's observations? |00:15 |---- |---- |colspan="4"|<big>'''Thursday 19 December 2019'''</big> |---- |09:30 |Gerry Gilmore |The next OPTICON opportunity [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GerryGilmore.pdf PDF] |00:20 |---- |09:50 |Gudrun Pebody |the OPTICON-RadioNet PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/GudrunPebody.pdf PDF] |00:15 |---- |10:05 |John Davies |(remote) TNA in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JohnDavies.pdf PDF] |00:15 |---- |10:20 |David Buckley |Transient astronomy in South Africa [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/DavidBuckley.pdf PDF] |00:25 |---- |10:45 |Marco Lam |Cross-platform automated spectral data reduction application [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcoLam.pdf PDF] |00:15 |---- |'''11:00''' |'''Coffee break ''' | |00:30 |---- |11:30 |Pawel Zieliński |Cambrigde Photometric Calibration Server 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PawelZielinski.pdf PDF] |00:15 |---- |11:45 |Przemysław Mikołajczyk |CCDPhot​ - an engine behind CPCS 2.0 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/PrzemekMikolajczyk.pdf PDF] |00:15 |---- |12:00 |Lukasz Wyrzykowski |OPTICON Time-Domain Network and its future including Black Hole TOM presentation [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/LukaszWyrzykowski.pdf PDF] |00:25 |---- |12:25 |Iair Arcavi |Rapid Robotic Followup of Transients [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/IairArcavi.pdf PDF] |00:25 |---- |'''12:50''' |'''Lunch break ''' | |01:10 |---- |14:00 |Rob Beswick |(remote) Radio Time Domain in the new PILOT [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/RobBeswick.pdf PDF] |00:20 |---- |14:20 |Marcin Gawroński |Radio observations in the era of time-domain astronomy [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MarcinGawronski.pdf PDF] |00:20 |---- |14:40 |''Discussion '' |''new OPTICON discussion'' |00:50 |---- |'''15:30''' |'''Coffee break ''' |'''Workshop photo''' |00:30 |---- |16:00 |Cosimo Inserra |ePESSTO+: the advanced Public ESO Spectroscopic Survey of Transient Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/CosimoInserra.pdf PDF] |00:30 |---- |16:30 |Mariusz Gromadzki |New types of transients in the era of all-sky surveys [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MariuszGromadzki.pdf PDF] |00:15 |---- |16:45 |Nada Ihanec |Nuclear transients in Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/NadaIhanec.pdf PDF] |00:15 |---- |17:00 |Mateusz Bronikowski |Identification of overluminous Gaia Alerts using photo-z catalogues [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/MateuszBronikowski.pdf PDF] |00:15 |---- |17:15 |Katja Bricman |Observing TDEs in the era of LSST [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KatjaBricman.pdf PDF] |00:15 |---- |'''20:00''' |'''Workshop Dinner''' | | |---- |---- |colspan="4"|<big>'''Friday 20 December 2019'''</big> |---- |09:30 |Zofia Kaczmarek |The search for IMBHs in Gaia: new simulations and results [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ZofiaKaczmarek.pdf PDF] |00:15 |---- |09:45 |Algita Stankevičiūtė |Atmospheric Turbulence challenges for hunting Black Holes with ground based telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AlgitaStankeviciute.pdf PDF] |00:15 |---- |10:00 |Kotryna Siskauskaite |Microlensing through binary black holes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KotrynaSiskauskaite.pdf PDF] |00:15 |---- |10:15 |Katarzyna Kruszyńska |Highlights from Microlensing events found in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KatarzynaKruszynska.pdf PDF] |00:20 |---- |10:35 |Krzysztof Rybicki |Gaia18bmt and Gaia19bld - highlights from microlensing alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/KrzysztofRybicki.pdf PDF] |00:20 |---- |'''10:55''' |'''Coffee break ''' | |00:35 |---- |11:30 |Agnieszka Gurgul |Polarimetric measurements of microlensing events; Solaris network of autonomous telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/AgnieszkaGurgul.pdf PDF] |00:20 |---- |11:50 |Tolga Güver |Istanbul University Observatory : IST60 as a Robotic Telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/TolgaGuver.pdf PDF] |00:15 |---- |12:05 |Nariman Ismailov |On the observational equipments in visual range at the Shamakhy Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/NarimanIsmailov.pdf PDF] |00:15 |---- |12:20 |Oliwia Ziółkowska |Loiano and Aristarchos in OPTICON [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/OliwiaZiolkowska.pdf PDF] |00:15 |---- |12:35 |Staszek Zola |Followup observations of Gaia alerts with SKYNET robotic telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/StaszekZola.pdf PDF] |00:15 |---- |12:50 |Erika Pakstiene |Stellar variability analysis at Molėtai Astronomical Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/ErikaPakstiene.pdf PDF] |00:15 |---- |13:05 |Justas Zdanavičius |Gaia alerts observation at Molėtai Astronomical Observatory [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2019/JustasZdanavicius.pdf PDF] |00:15 |---- |'''13:20''' |'''Lunch break ''' | |00:55 |---- |14:15 |''Discussion'' |"Technical issues, comments'' | |---- |15:15 |'''end of the workshop ''' | | |---- |} ''last update: 21/12/2019 06:14'' ---- The Social Dinner will be held on '''Thursday 19th December''' at 20:00.<br /> On Saturday, 21.Dec, there will be an interesting social event/trip, so if you can, please stay a bit longer! More details on the Social programme and the trips are available under [[Workshop2019:logistics|Logistics pages]] aef517cb74809d9403aab759acc6a93b041d7709 0 307 2529 2407 2019-12-19T13:04:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) === Workshop 2019 Photo === [[File:workshop2019_small.jpg]] 42a1c9a1a56947a80636ae3598f121eb581ade22 2531 2529 2019-12-19T13:05:16Z Gsawgwikiadmin 1 /* Workshop 2019 Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) === Workshop 2019 Photo === [[File:workshop2019.jpg]] b2df1b9ea2b24e481581d6f2dbf1c04d619c09f3 2533 2531 2019-12-19T13:06:47Z Gsawgwikiadmin 1 /* Workshop 2019 Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) === Workshop 2019 Photo === [[File:workshop2019.jpg|200px]] 14a198b63003f1aa04c912ff7f5540eaf9bb0cac 2534 2533 2019-12-19T13:06:54Z Gsawgwikiadmin 1 /* Workshop 2019 Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) === Workshop 2019 Photo === [[File:workshop2019.jpg]] b2df1b9ea2b24e481581d6f2dbf1c04d619c09f3 2535 2534 2019-12-19T13:07:21Z Gsawgwikiadmin 1 /* Workshop 2019 Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) === Workshop 2019 Photo === [[File:workshop2019.jpg|200px]] 14a198b63003f1aa04c912ff7f5540eaf9bb0cac 2536 2535 2019-12-19T13:07:31Z Gsawgwikiadmin 1 /* Workshop 2019 Photo */ wikitext text/x-wiki == Welcome! == [[File:Poster2019-small.png|right|450px|poster2019]] '''The tenth OPTICON Gaia Science Alerts workshop will be held in [[Workshop2019:logistics | Catania, Sicily, 18-20 December 2019]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2019:rationale|Rationale]] * [[workshop2019:agenda|Agenda]] * [[workshop2019:registration|Registration]] * [[workshop2019:logistics|Logistic information]] * [[workshop2019:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Giuseppe Leto (INAF-OACT) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Flavia Calderone (INAF-OACT) * Giancarlo Bellassai (INAF-OACT) * Ricardo Zanmar Sanchez (INAF-OACT) === Workshop 2019 Photo === [[File:workshop2019.jpg|800px]] 89aac87cc605ccd70191bea75693ead8b1b441ec 6 330 2530 2019-12-19T13:04:39Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 331 2532 2019-12-19T13:05:56Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 1 2545 2373 2020-03-06T14:02:48Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, Cambridge, UK, 22-25 September 2020]]</Big>''' </center> ---- <center> [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 2eac6e73b9f212f899ab3af5fbd40a7af14987e0 2555 2545 2020-08-11T06:45:30Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, Virtual, 28-30 September 2020]]</Big>''' </center> ---- <center> [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 2778b85faa0ca07a49373961b1b7f91ba3211fea 0 332 2546 2020-03-06T14:05:25Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held in Workshop2020:logistics | Cambridge..." wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2020:logistics | Cambridge, UK, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) d52ccc78c51b08f6546a181a309d469a0df527ed 2548 2546 2020-03-23T12:19:44Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED''' '''The eleventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2020:logistics | Cambridge, UK, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) ad45eab25cd0f6dafe2cd304f66e466853908899 2549 2548 2020-03-23T12:19:59Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2020:logistics | Cambridge, UK, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) ca251a4a33531ac409c7007d51b18e6d9d835818 2552 2549 2020-08-11T06:35:29Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2020:logistics | virtually, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 87bf02803065d8c72b1d2ed01bd09b3fcf6a4da4 2553 2552 2020-08-11T06:35:32Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2020:logistics | Cambridge, UK, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) ca251a4a33531ac409c7007d51b18e6d9d835818 2554 2553 2020-08-11T06:35:48Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held in [[Workshop2020:logistics | virtually, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 87bf02803065d8c72b1d2ed01bd09b3fcf6a4da4 8 3 2547 2375 2020-03-06T14:09:19Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2020 **workshop2020:main|Main Workshop Page **workshop2020:rationale|Rationale **workshop2020:agenda|Program **workshop2020:registration|Participants and Registration **workshop2020:logistics|Logistics *workshop 2019 **workshop2019:main|Main Workshop Page **workshop2019:agenda|Archive of presentations *workshop 2018 **workshop2018:main|Main Workshop Page **workshop2018:agenda|Archive of presentations *workshop 2017 **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 4d225fd77ddc04cedc56aed5877b5476d81aa034 0 200 2550 2356 2020-03-24T15:46:41Z Gsawgwikiadmin 1 /* Data Policy */ wikitext text/x-wiki The main address of the server is: http://gsaweb.ast.cam.ac.uk/followup == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. Updated December 2016 by LW. == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org = Data Policy = If you use any of the data from the Calibration Server in your publication, please acknowledge it with the following text: '''We acknowledge the use of the Cambridge Photometric Calibration Server (http://gsaweb.ast.cam.ac.uk/followup), developed by Sergey Koposov and maintained by Lukasz Wyrzykowski, Arancha Delgado, Pawel Zielinski, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890 (OPTICON).''' <big>Also note that if the data from the CPCS is essential for the paper, please include the observers as co-authors.</big> 3f43056281ba024447cae44c40918c2629405c8f 0 332 2556 2554 2020-08-11T06:45:47Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | virtually, 28-30 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 5d278347f3ededd6a50f2f1ddc8769ca000ae25e 2557 2556 2020-08-11T06:46:14Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | virtually, 21-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 6acf730bc218ec4fe5c3767df2be9a01673d163f 2559 2557 2020-08-11T06:46:54Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | virtually, 22-25 September 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 3669f332f2946b49caf83d2262de1f3bbc828518 2561 2559 2020-09-04T09:44:00Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | virtually, in Autumn 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 2cc1d6f3d5cf7a805e0b27ca3e910759b7b7ffd6 2564 2561 2020-11-11T05:49:05Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 14-18 December 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] * [[workshop2020:poster|Workshop's poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 6413c1a28f03834809eacdead28716e5b1d82230 2581 2564 2020-11-11T08:43:35Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 14-18 December 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Simon Hodgkin (Cambridge) * Lukasz Wyrzykowski (Warsaw) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) bf5a088c5982973c910cfa3f46f74386bfd83ddf 2582 2581 2020-11-11T08:44:08Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 14-18 December 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 6b1354bcb74254d48e4dc753b0d7be51b0301345 2583 2582 2020-11-12T16:48:47Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 14-18 December 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) e575e57767b50e40defcd51aa88dd103bca594ab 2584 2583 2020-11-14T08:16:09Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] <big>'''NOTE: THE DATE IS NOT YET CONFIRMED! WE WILL KEEP YOU INFORMED'''</big> '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online in early January 2020]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) e58b9281ecac42590e8a5d0ad94669aae14d9e1b 2587 2584 2020-11-16T08:00:02Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]].''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 9fbd517b3878d8155087764b4ed142b95de852d5 2588 2587 2020-11-16T08:00:15Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistic information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 8d40a55ed51adc240660c5762358fa71b23bfc9b 2590 2588 2020-11-16T08:12:43Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) 8c1a882fc13799398223f4066495dc4902340022 2591 2590 2020-11-30T11:59:48Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Mascoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) f4c4bdc74389a2ae2ab9072279b0cf2ad2edcf91 2592 2591 2020-11-30T12:03:46Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. 0f69561bb034e8d889f8fa09209cb200f9c634e3 2601 2592 2020-12-12T07:33:57Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[Media:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. 306a92c07c93a0e21962a44ea80c56add1968340 0 1 2558 2555 2020-08-11T06:46:42Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, Virtual, 22-25 September 2020]]</Big>''' </center> ---- <center> [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 7addaddb190324e3ddc0bf7be31c9423ddb76e99 2560 2558 2020-09-04T09:43:42Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, Virtual, TBD, Autumn 2020]]</Big>''' </center> ---- <center> [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 0629915b3d064113731ac597659b23d5f25bc116 2562 2560 2020-11-11T05:48:16Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, Virtual, 14-18 December 2020]]</Big>''' </center> ---- <center> [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 2ad6e31b793fedad2f957f6b851f87f2b97ffdea 2563 2562 2020-11-11T05:48:26Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, On-line, 14-18 December 2020]]</Big>''' </center> ---- <center> [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 68d6c5953209e1b2f5014169fda1467928f9cabe 0 333 2565 2020-11-11T05:52:44Z Gsawgwikiadmin 1 Created page with "The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for..." wikitext text/x-wiki The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for interactions with the speakers and taking part in the discussions. We will also stream and record the presentations on '''YouTube'''. d32419975899269bc7a17ff2190936b3b7cb7aca 2603 2565 2021-01-07T06:17:54Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for interactions with the speakers and taking part in the discussions. We will also stream and record the presentations on '''YouTube'''. == Code of Conduct == Every participant of the ''11th OPTICON Gaia Science Alerts Workshop'' is asked to follow the rules below: * Behave professionally. Harassment and sexist, racist, or exclusionary comments or jokes are not appropriate. Harassment includes sustained disruption of talks or other events, inappropriate physical contact, sexual attention or innuendo, deliberate intimidation, stalking, and photography or recording of an individual without consent. It also includes offensive comments related to individual characteristics, for example, age, gender, sexual orientation, disability, physical appearance, race, nationality or religion. * All communication should be appropriate for a professional audience including people of many different backgrounds. Sexual or sexist language and imagery are not appropriate. * Be respectful and do not insult or put down other attendees or facilitators of the event. Critique ideas, not people. * Should a participant witness events of bullying, harassment or aggression, we recommend that they approach the affected person to show support and check how they are. The witness may also wish to suggest that the person report the inappropriate behaviour. However, it is up to the affected person alone whether or not they wish to report it. * If participants wish to share photos of a speaker on social media, we strongly recommend that they first get the speaker’s permission. Participants may also share the contents of talks/slides via social media unless speakers have asked that specific details/slides not be shared. * Participants can report any violation of these guidelines to any member of Workshop Organizing Committee (WOC) in confidence. If asked to stop inappropriate behaviour participants are expected to comply immediately and, in serious cases, may be asked to leave the event. WOC will not tolerate retaliation against anyone reporting violations of this code of conduct. * These rules are in line with the [https://www.iau.org/static/archives/announcements/pdf/ann16007a.pdf IAU anti-harassment guidelines] and the [https://eas.unige.ch//documents/EAS_Ethics_Statement.pdf EAS ethics statement]. 4e823e66e2a2f534207903ad52d7c6a933ef4473 2604 2603 2021-01-07T06:21:55Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for interactions with the speakers and taking part in the discussions. The talks will be recorded and made public on '''YouTube''' unless a speaker clearly objects to this. We will also use [https://www.wonder.me/ Wonder] platform for communication outside of the sessions. The channel will be open 24h and participants are invited to use it for informal discussions and smaller group meetings throughout the entire week of the workshop. == Code of Conduct == Every participant of the ''11th OPTICON Gaia Science Alerts Workshop'' is asked to follow the rules below: * Behave professionally. Harassment and sexist, racist, or exclusionary comments or jokes are not appropriate. Harassment includes sustained disruption of talks or other events, inappropriate physical contact, sexual attention or innuendo, deliberate intimidation, stalking, and photography or recording of an individual without consent. It also includes offensive comments related to individual characteristics, for example, age, gender, sexual orientation, disability, physical appearance, race, nationality or religion. * All communication should be appropriate for a professional audience including people of many different backgrounds. Sexual or sexist language and imagery are not appropriate. * Be respectful and do not insult or put down other attendees or facilitators of the event. Critique ideas, not people. * Should a participant witness events of bullying, harassment or aggression, we recommend that they approach the affected person to show support and check how they are. The witness may also wish to suggest that the person report the inappropriate behaviour. However, it is up to the affected person alone whether or not they wish to report it. * If participants wish to share photos of a speaker on social media, we strongly recommend that they first get the speaker’s permission. Participants may also share the contents of talks/slides via social media unless speakers have asked that specific details/slides not be shared. * Participants can report any violation of these guidelines to any member of Workshop Organizing Committee (WOC) in confidence. If asked to stop inappropriate behaviour participants are expected to comply immediately and, in serious cases, may be asked to leave the event. WOC will not tolerate retaliation against anyone reporting violations of this code of conduct. * These rules are in line with the [https://www.iau.org/static/archives/announcements/pdf/ann16007a.pdf IAU anti-harassment guidelines] and the [https://eas.unige.ch//documents/EAS_Ethics_Statement.pdf EAS ethics statement]. 5b1d1573f20669c74b69e78632146669f17adc42 2605 2604 2021-01-07T06:23:26Z Gsawgwikiadmin 1 wikitext text/x-wiki == Connection details == The links will be provided to the registered participants only. The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for interactions with the speakers and taking part in the discussions. The talks will be recorded and made public on '''YouTube''' unless a speaker clearly objects to this. We will also use [https://www.wonder.me/ Wonder] platform for communication outside of the sessions. The channel will be open 24h and participants are invited to use it for informal discussions and smaller group meetings throughout the entire week of the workshop. There is also a Slack Workspace named Black Hole TOM Workspace, we encourage participants to use that medium during and after the workshop for further communication. == Code of Conduct == Every participant of the ''11th OPTICON Gaia Science Alerts Workshop'' is asked to follow the rules below: * Behave professionally. Harassment and sexist, racist, or exclusionary comments or jokes are not appropriate. Harassment includes sustained disruption of talks or other events, inappropriate physical contact, sexual attention or innuendo, deliberate intimidation, stalking, and photography or recording of an individual without consent. It also includes offensive comments related to individual characteristics, for example, age, gender, sexual orientation, disability, physical appearance, race, nationality or religion. * All communication should be appropriate for a professional audience including people of many different backgrounds. Sexual or sexist language and imagery are not appropriate. * Be respectful and do not insult or put down other attendees or facilitators of the event. Critique ideas, not people. * Should a participant witness events of bullying, harassment or aggression, we recommend that they approach the affected person to show support and check how they are. The witness may also wish to suggest that the person report the inappropriate behaviour. However, it is up to the affected person alone whether or not they wish to report it. * If participants wish to share photos of a speaker on social media, we strongly recommend that they first get the speaker’s permission. Participants may also share the contents of talks/slides via social media unless speakers have asked that specific details/slides not be shared. * Participants can report any violation of these guidelines to any member of Workshop Organizing Committee (WOC) in confidence. If asked to stop inappropriate behaviour participants are expected to comply immediately and, in serious cases, may be asked to leave the event. WOC will not tolerate retaliation against anyone reporting violations of this code of conduct. * These rules are in line with the [https://www.iau.org/static/archives/announcements/pdf/ann16007a.pdf IAU anti-harassment guidelines] and the [https://eas.unige.ch//documents/EAS_Ethics_Statement.pdf EAS ethics statement]. d6ee5cba2273c58c147ea45af1c98d10c4d4478a 0 334 2566 2020-11-11T06:12:49Z Gsawgwikiadmin 1 Created page with "The workshop will be held for about 3h every of 5 days. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be abl..." wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. f791573e44ee43668b7f2ce803eaaa1d02efdaa6 2567 2566 2020-11-11T06:14:39Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. ---- {| class="wikitable" | |Monday 14.Dec |- |Tuesday 15.Dec |- |Wednesday 16.Dec |- |Thursday 17.Dec |- |Friday 18.Dec |- ---- 6c3a4ce3c7f68c503c848b59d7c3ee908f3d130e 2568 2567 2020-11-11T06:15:16Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. ---- {| class="wikitable" | |Monday 14.Dec |---- |Tuesday 15.Dec |---- |Wednesday 16.Dec |---- |Thursday 17.Dec |---- |Friday 18.Dec |---- |} ---- 4d71274cb932b62a04623bb745eac04ab3359695 2569 2568 2020-11-11T06:15:27Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. ---- {| class="wikitable" |---- |Monday 14.Dec |---- |Tuesday 15.Dec |---- |Wednesday 16.Dec |---- |Thursday 17.Dec |---- |Friday 18.Dec |---- |} ---- d684b15859ba595a3ac9b024aad1fff010e1fbdc 2570 2569 2020-11-11T06:36:24Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. ---- {| class="wikitable" |---- |Monday 14.Dec |---- |Tuesday 15.Dec |---- |Wednesday 16.Dec |---- |Thursday 17.Dec |---- |Friday 18.Dec |---- |} ---- b862c3a690cc4d3c0591be4293680b415f79f08e 2571 2570 2020-11-11T06:43:54Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png]] ---- {| class="wikitable" |---- |Monday 14.Dec |---- |Tuesday 15.Dec |---- |Wednesday 16.Dec |---- |Thursday 17.Dec |---- |Friday 18.Dec |---- |} ---- 790c8939143a842be03411972d6ba20a701de553 2573 2571 2020-11-11T06:45:42Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |Monday 14.Dec |---- |Tuesday 15.Dec |---- |Wednesday 16.Dec |---- |Thursday 17.Dec |---- |Friday 18.Dec |---- |} ---- 31f2c26a74aeb0c2e09e0bc7742f18df57baac18 2574 2573 2020-11-11T07:27:42Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |Europe |New York |Los Angeles |---- |Monday 14.Dec | 2pm | (+1d ) 2am | 11pm | 7:30pm | 3pm | 2pm | 9am | 6am |---- |Tuesday 15.Dec |9am |10pm |6pm |2:30pm |10am |9am |4am |1am |---- |Wednesday 16.Dec |5pm |(+1d) 6am |(+1d) 2am |10:30pm |6pm |5pm |12pm |9am |---- |Thursday 17.Dec |9am |10pm |6pm |2:30pm |10am |9am |4am |1am |---- |Friday 18.Dec |---- |2pm |(+1d)3am |11pm |7:30pm |3pm |2pm |9am |6am |} ---- 4241b0c677530a735fbfff10264e6259c60fbd64 2575 2574 2020-11-11T07:27:59Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |Europe |New York |Los Angeles |---- |Monday 14.Dec | 2pm | (+1d ) 2am | 11pm | 7:30pm | 3pm | 2pm | 9am | 6am |---- |Tuesday 15.Dec |9am |10pm |6pm |2:30pm |10am |9am |4am |1am |---- |Wednesday 16.Dec |5pm |(+1d) 6am |(+1d) 2am |10:30pm |6pm |5pm |12pm |9am |---- |Thursday 17.Dec |9am |10pm |6pm |2:30pm |10am |9am |4am |1am |---- |Friday 18.Dec |2pm |(+1d)3am |11pm |7:30pm |3pm |2pm |9am |6am |---- |} ---- 4e6552ce364e6d011903d638b307666f9566d288 2576 2575 2020-11-11T07:28:25Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |Europe |UK |New York |Los Angeles |---- |Monday 14.Dec | 2pm | (+1d ) 2am | 11pm | 7:30pm | 3pm | 2pm | 9am | 6am |---- |Tuesday 15.Dec |9am |10pm |6pm |2:30pm |10am |9am |4am |1am |---- |Wednesday 16.Dec |5pm |(+1d) 6am |(+1d) 2am |10:30pm |6pm |5pm |12pm |9am |---- |Thursday 17.Dec |9am |10pm |6pm |2:30pm |10am |9am |4am |1am |---- |Friday 18.Dec |2pm |(+1d)3am |11pm |7:30pm |3pm |2pm |9am |6am |---- |} ---- 65ad308b2586f80469e941dccac3bc8b3d7bc29c 2577 2576 2020-11-11T07:29:16Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. There will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 14.Dec |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 15.Dec |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 16.Dec |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 17.Dec |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 18.Dec |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- 1b883a45549217c529b8214f0c83f59e7d45f932 2578 2577 2020-11-11T07:29:58Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. During the registration there will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 14.Dec |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 15.Dec |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 16.Dec |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 17.Dec |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 18.Dec |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- c8ace33045c3ec9e89c28412cb56265ec4ed4e8e 2585 2578 2020-11-16T07:00:34Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. During the registration there will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- 2e637441bfdd64a109229f775c492f0f7afd22f5 2602 2585 2020-12-28T07:11:53Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. During the registration, there will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool. The link to Wonder Room will be provided to the registered participants. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- e0658200d5e76f94622ec8836164d7e062345086 6 335 2572 2020-11-11T06:44:13Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2586 2572 2020-11-16T07:59:25Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:SchedulePoll.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 336 2579 2020-11-11T08:22:39Z Gsawgwikiadmin 1 Created page with "= <big>Registration is now open!</big> = <big>'''[https://forms.gle/oukbNW3M8wewRJVB8 CLICK HERE FOR THE REGISTRATION FORM]'''</big>" wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/oukbNW3M8wewRJVB8 CLICK HERE FOR THE REGISTRATION FORM]'''</big> b27bf6954a95b309ffc18dc0418acc470a7679de 2580 2579 2020-11-11T08:26:23Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> a35d245fa741f2bf024febb5a92d6e306a8a84a4 2589 2580 2020-11-16T08:03:02Z Gsawgwikiadmin 1 /* Registration is now open! */ wikitext text/x-wiki = <big>Registration is now open!</big> = The requests for talks will be accepted until '''January 10th 2021'''. <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> 773f13d8595536b45571d344ebf1caa95c8f1312 2593 2589 2020-12-01T13:18:13Z Gsawgwikiadmin 1 /* Registration is now open! */ wikitext text/x-wiki = <big>Registration is now open!</big> = The requests for talks will be accepted until '''January 10th 2021'''. <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. 1a681ff05f90f1e2d2d4c35f6e41d016c385c59e 2594 2593 2020-12-08T13:20:23Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = The requests for talks will be accepted until '''January 10th 2021'''. ''After the registration process, you will be asked to select your preferred time slot. Please select as many as possible for different days and times. Please check the [[Workshop2020:agenda agenda page]] for more details.'' <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. fc7782f258ca0ab97cda34c6ca61cd23fcd85d36 2595 2594 2020-12-08T13:20:33Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = The requests for talks will be accepted until '''January 10th 2021'''. ''After the registration process, you will be asked to select your preferred time slot. Please select as many as possible for different days and times. Please check the [[Workshop2020:agenda|agenda page]] for more details.'' <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. 52d7b3fb49f2352229f738dd62ac1a610a1d1275 0 337 2596 2020-12-09T06:01:45Z Gsawgwikiadmin 1 Created page with "* Gaia and Gaia Alerts ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometri..." wikitext text/x-wiki * Gaia and Gaia Alerts ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometric data, and Gaia Photometric Science Alerts continues as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. * Gaia Alerts Science 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 * Follow-up At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. * Workshop's promise 
 The forthcoming Gaia Alerts Workshop, the 11th in the series, will be an opportunity to learn about the current state (and future plans for) Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia Alerts, and we will explore the scientific potential of the programme. * Multimessenger time-domain
 In particular, we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increase the scientific output of surveys and follow-up observations in the multi-messenger era. 
 * Logistics The workshop will be held on Zoom Platform and will last for about 3h every day at different times of the day so that we can accommodate attendees from different time-zones. During the registration process, you will be asked to select the most suitable time and day for your presentation. Please note the number of slots available for talks is limited. You will be informed if your talk was accepted by the WOC. 7a880502f8c528d08b671ea05ba63e976ec63ef0 2597 2596 2020-12-09T06:02:34Z Gsawgwikiadmin 1 wikitext text/x-wiki == Gaia and Gaia Alerts ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometric data, and Gaia Photometric Science Alerts continues as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. == Gaia Alerts Science 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 == Follow-up At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. == Workshop's promise 
 The forthcoming Gaia Alerts Workshop, the 11th in the series, will be an opportunity to learn about the current state (and future plans for) Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia Alerts, and we will explore the scientific potential of the programme. == Multimessenger time-domain
 In particular, we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increase the scientific output of surveys and follow-up observations in the multi-messenger era. 
 == Logistics The workshop will be held on Zoom Platform and will last for about 3h every day at different times of the day so that we can accommodate attendees from different time-zones. During the registration process, you will be asked to select the most suitable time and day for your presentation. Please note the number of slots available for talks is limited. You will be informed if your talk was accepted by the WOC. c1d82ad3de366085d2f9c77d80dc13448e32407f 2598 2597 2020-12-09T06:03:06Z Gsawgwikiadmin 1 wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometric data, and Gaia Photometric Science Alerts continues as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Gaia Alerts Science === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 11th in the series, will be an opportunity to learn about the current state (and future plans for) Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia Alerts, and we will explore the scientific potential of the programme. === Multimessenger time-domain
 === In particular, we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increase the scientific output of surveys and follow-up observations in the multi-messenger era. 
 === Logistics === The workshop will be held on Zoom Platform and will last for about 3h every day at different times of the day so that we can accommodate attendees from different time-zones. During the registration process, you will be asked to select the most suitable time and day for your presentation. Please note the number of slots available for talks is limited. You will be informed if your talk was accepted by the WOC. 7c0bbd3dd40c5c0450c9ad68966cbb422f7466f1 6 338 2599 2020-12-12T07:27:51Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 339 2600 2020-12-12T07:30:35Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 333 2606 2605 2021-01-07T06:23:49Z Gsawgwikiadmin 1 wikitext text/x-wiki == Connection details == The links will be provided to the registered participants only. The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for interactions with the speakers and taking part in the discussions. The talks will be recorded and made public on '''YouTube''' unless a speaker clearly objects to this. We will also use [https://www.wonder.me/ Wonder] platform for communication outside of the sessions. The channel will be open 24h and participants are invited to use it for informal discussions and smaller group meetings throughout the entire week of the workshop. There is also a '''Slack workspace''' named '''Black Hole TOM Workspace''', we encourage participants to use that medium during and after the workshop for further communication. == Code of Conduct == Every participant of the ''11th OPTICON Gaia Science Alerts Workshop'' is asked to follow the rules below: * Behave professionally. Harassment and sexist, racist, or exclusionary comments or jokes are not appropriate. Harassment includes sustained disruption of talks or other events, inappropriate physical contact, sexual attention or innuendo, deliberate intimidation, stalking, and photography or recording of an individual without consent. It also includes offensive comments related to individual characteristics, for example, age, gender, sexual orientation, disability, physical appearance, race, nationality or religion. * All communication should be appropriate for a professional audience including people of many different backgrounds. Sexual or sexist language and imagery are not appropriate. * Be respectful and do not insult or put down other attendees or facilitators of the event. Critique ideas, not people. * Should a participant witness events of bullying, harassment or aggression, we recommend that they approach the affected person to show support and check how they are. The witness may also wish to suggest that the person report the inappropriate behaviour. However, it is up to the affected person alone whether or not they wish to report it. * If participants wish to share photos of a speaker on social media, we strongly recommend that they first get the speaker’s permission. Participants may also share the contents of talks/slides via social media unless speakers have asked that specific details/slides not be shared. * Participants can report any violation of these guidelines to any member of Workshop Organizing Committee (WOC) in confidence. If asked to stop inappropriate behaviour participants are expected to comply immediately and, in serious cases, may be asked to leave the event. WOC will not tolerate retaliation against anyone reporting violations of this code of conduct. * These rules are in line with the [https://www.iau.org/static/archives/announcements/pdf/ann16007a.pdf IAU anti-harassment guidelines] and the [https://eas.unige.ch//documents/EAS_Ethics_Statement.pdf EAS ethics statement]. 74057a552d7da32f6052553de4d4a37b7921ef2d 2619 2606 2021-01-13T16:19:14Z Gsawgwikiadmin 1 /* Code of Conduct */ wikitext text/x-wiki == Connection details == The links will be provided to the registered participants only. The meeting will be held on '''Zoom''' platform. Please install the Client from [https://zoom.us/download]. Alternatively, Zoom can be run from a browser. Zoom will allow for interactions with the speakers and taking part in the discussions. The talks will be recorded and made public on '''YouTube''' unless a speaker clearly objects to this. We will also use [https://www.wonder.me/ Wonder] platform for communication outside of the sessions. The channel will be open 24h and participants are invited to use it for informal discussions and smaller group meetings throughout the entire week of the workshop. There is also a '''Slack workspace''' named '''Black Hole TOM Workspace''', we encourage participants to use that medium during and after the workshop for further communication. == Code of Conduct == Every participant of the ''11th OPTICON Gaia Science Alerts Workshop'' is asked to follow the rules below: * Behave professionally. Harassment and sexist, racist, or exclusionary comments or jokes are not appropriate. Harassment includes sustained disruption of talks or other events, inappropriate physical contact, sexual attention or innuendo, deliberate intimidation, stalking, and photography or recording of an individual without consent. It also includes offensive comments related to individual characteristics, for example, age, gender, sexual orientation, disability, physical appearance, race, nationality or religion. * All communication should be appropriate for a professional audience including people of many different backgrounds. Sexual or sexist language and imagery are not appropriate. * Be respectful and do not insult or put down other attendees or facilitators of the event. Critique ideas, not people. * Should a participant witness events of bullying, harassment or aggression, we recommend that they approach the affected person to show support and check how they are. The witness may also wish to suggest that the person report the inappropriate behaviour. However, it is up to the affected person alone whether or not they wish to report it. * If participants wish to share photos of a speaker on social media, we strongly recommend that they first get the speaker’s permission. Participants may also share the contents of talks/slides via social media unless speakers have asked that specific details/slides not be shared. * Participants can report any violation of these guidelines to any member of Workshop Organizing Committee (WOC) in confidence. If asked to stop inappropriate behaviour participants are expected to comply immediately and, in serious cases, may be asked to leave the event. WOC will not tolerate retaliation against anyone reporting violations of this code of conduct. * These rules are in line with the [https://www.iau.org/static/archives/announcements/pdf/ann16007a.pdf IAU anti-harassment guidelines] and the [https://eas.unige.ch//documents/EAS_Ethics_Statement.pdf EAS ethics statement]. * Anonymous use of Zoom/WonderMe platforms is not allowed. Please rename your avatar so it refers to your First and Last Name. 6b5a814845b93173c16ee8b9251168e3a5ced8a0 0 336 2607 2595 2021-01-11T14:17:35Z Gsawgwikiadmin 1 wikitext text/x-wiki = <big>Registration is now open!</big> = The requests for talks is now closed. However, if you feel you still need to register, please email Lukasz Wyrzykowski lw at astrouw.edu.pl. <!--- ''After the registration process, you will be asked to select your preferred time slot. Please select as many as possible for different days and times. Please check the [[Workshop2020:agenda|agenda page]] for more details.'' <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. ---> bcedf23e13876721622013d8942b4685f05334e5 2620 2607 2021-01-13T16:51:22Z Gsawgwikiadmin 1 wikitext text/x-wiki The requests for talks is now closed. However, if you feel you still need to register, please email Lukasz Wyrzykowski lw at astrouw.edu.pl. <!--- ''After the registration process, you will be asked to select your preferred time slot. Please select as many as possible for different days and times. Please check the [[Workshop2020:agenda|agenda page]] for more details.'' <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. ---> == Registered participants == # Karsten Brogaard Stellar astrophysics Centre, Aarhus University, Denmark # Rachel Street Las Cumbres Observatory, USA # Josep Manel Carrasco Universitat de Barcelona # Marco Lam Tel Aviv University, Israel # Akihiko Fukui The University of Tokyo, Japan # Mateusz Bronikowski Astronomical Observatory, University of Warsaw, Poland # Dmitry Blinov Institute of Astrophysics, FORTH, Greece # Dirk Froebrich University of Kent # Charles Galdies University of Malta # Morgan Fraser University College Dublin, Ireland # Nikolaos Mandarakas University of Crete, Physics Department, Greece # Iair Arcavi Tel Aviv University, Israel # Malhar Kendurkar Prince George Astronomical Observatory, Canada # Nami Mowlavi Department of Astronomy, University of Geneva, CH # Klaas Wiersema University of Warwick, UK # Hasan H. Esenoglu Istanbul University Observatory, University Central Campus, Beyazit, Fatih, Istanbul, Turkey # John Davies OPTICON, UK # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław, Poland # Fraser Lewis Faulkes Telescope Project & National Schools' Observatory, UK # Maja Jabłońska University of Warsaw, Poland # Szymon Kozlowski Astronomical Observatory, University of Warsaw , Poland # Katarzyna Kruszyńska Astronomical Observatory, University of Warsaw, Poland # Pawel Zielinski Astronomical Observatory, University of Warsaw, Poland # Algita Stankevičiūtė Astronomical observatory of the University of Warsaw, Poland # Gaspar Bakos Princeton University, USA # Mariusz Gromadzki Astronomical Observatory, University of Warsaw, Poland # Nariman Ismailov Shamakhi Astrophysical Observatory, Azerbeijan # Benny Trakhtenbrot Tel Aviv University, Israel # Tsvi Piran The Hebrew University , Israel # Ashish Mahabal Caltech, USA # Ilknur Gezer Warsaw University Astronomical Observatory, Poland # Gábor Marton CSFK Konkoly Observatory, Hungary # Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungary # Michel Dennefeld IAP-Paris, France # Goran Damljanovic Astronomical Observatory, Serbia # Jaroslav Merc Astronomical Institute of Charles University in Prague, Czechia # Roberto Alexander Cerviño Department of Data Science, Faculty of Computer Science, Multimedia and Telecommunications, Universitat Oberta de Catalunya # Michał Siwak Konkoly Observatory, Hungary # Nada Ihanec Astronomical Observatory, University of Warsaw, Poland # William Thuillot Paris Observatory / IMCCE, France # Ruta Urbonaviciute Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Kris Rybicki Astronomical Observatory, University of Warsaw, Poland # Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University, Lithuania # Justas Zdanavičius Astronomical Observatory of the Vilnius University, Lithuania # Etienne Bachelet Las Cumbres Observatory, USA # Przemek Mroz California Institute of Technology, USA # Zofia Kaczmarek Warsaw University Astronomical Observatory, Poland # Agnieszka Słowikowska Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland # Maria Gabriela Navarro Sapienza / MAS / UNAB, Chile/Italy # Zuzanna Kostrzewa-Rutkowska Leiden Observatory, NL # Benito Marcote Joint Institute for VLBI ERIC (JIVE), NL # Artie Hatzes Thüringer Landessternwarte Tautenburg, Germany # Nicholas Rattenbury The University of Auckland, New Zeleand # Takahiro Sumi Osaka University, Japan # Gerry Gilmore IoA Cambridge, UK # Eran Ofek Weizmann Institute of Science, Israel # Simon Hodgkin University of Cambridge, UK # Harro Verkouter Joint Institute for VLBI in Europe, NL # Marzena Sniegowska Nicolaus Copernicus Astronomical Center Polish Academy of Sciences, Poland # Maria Jose Rain Universita' degli studi di Padova, Italy # Aayush Gautam Birendra Multiple Campus, Tribhuvan University, Nepal # Timur Şahin Akdeniz University, Turkey # László Szabados Konkoly Observatory, Hungary # Andrzej Pigulski University of Wrocław, Poland # Monika Kamińska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University, Poland # Stephen Brincat Flarestar Observatory (MPC:171); AAVSO # Krzysztof Kamiński Astronomical Observatory of Adam Mickiewicz University, Poland # Prasanta Kumar Nayak Tata Institute of Fundamental Research, Mumbai, India # Sepideh Eskandarlou Kharazmi university, Iran # Michał Żejmo Instytut Astronomii im. profesora Janusza Gila, Uniwersytet Zielonogórski, Poland # Yogesh Joshi Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, India # Lydia Makrygianni Tel Aviv University, Israel # Waldemar Ogloza Mt.Suhora Observatory, Cracow Pedagogical University, Poland # Laura Ruiz-Dern Department of Data Science, Faculty of Computer Science, Multimedia and Telecommunications, Universitat Oberta de Catalunya # Areg Mickaelian Byurakan Astrophysical Observatory (BAO), Armenia # Staszek Zola Astronomical Observatory, Jagiellonian University, Poland # Roberto Figuera Jaimes San Sebastian University, USA # Milena Ratajczak Astronomical Observatory, University of Warsaw, Poland # Salim Ansari ESA - ESTEC # Mike Garrett University of Manchester, UK # Franz-Josef Hambsch Vereniging Voor Sterrenkunde (VVS), Oostmeers 122 C, 8000 Brugge, Belgium # Ryszard Szczerba Nicolaus Copernicus Astronomical Center, Poland # Karolina Bąkowska N. Copernicus University, Poland # Emma Dodd Kapteyn, University of Groningen, NL # Siegfried Vanaverbeke astrolab IRIS observatory # Elahe Khalouei Sharif university of technology, Iran # Kotryna Siskauskaite Vilnius University, Lithuania # Ágnes Kóspál Konkoly Observatory, Budapest, Hungary # Péter Ábrahám Konkoly Observatory, Hungary # Aishwarya Selvaraj University of Manchester, UK # Sunkyung Park Konkoly Observatory, Hungary # Markus Hundertmark ARI, Zentrum für Astronomie, Universität Heidelberg, Germany # Erika Pakštienė Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Vytautas Čepas Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Seppo Mattila University of Turku, Finland # Lorenzo Rimoldini University of Geneva, CH # Krzysztof Nienartowicz ESA Gaia DPCG/CU7, Geneva, CH # Laurent Eyer Universit of Geneva, CH # Berry Holl Department of Astronomy, Geneva, CH # Shri Kulkarni Caltech, USA # Malgorzata van Leeuwen Institute of Astronomy, University of Cambridge, UK # Cristina Barbarino Tel Aviv University, IL # Simon Hodgkin Institute of Astronomy, University of Cambridge, UK # Mikołaj Kałuszyński Nicolaus Copernicus Astronomical Center, Poland # Timo Prusti ESA, NL # Guy Rixon IoA Cambridge, UK # Elme Breedt IoA, University of Cambridge, UK 777bca37d1cd6c42b2eca005b62f5eaaa3a5310d 2629 2620 2021-01-15T20:28:29Z Gsawgwikiadmin 1 wikitext text/x-wiki The requests for talks is now closed. However, if you feel you still need to register, please email Lukasz Wyrzykowski lw at astrouw.edu.pl. <!--- ''After the registration process, you will be asked to select your preferred time slot. Please select as many as possible for different days and times. Please check the [[Workshop2020:agenda|agenda page]] for more details.'' <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. ---> == Registered participants == # Karsten Brogaard Stellar astrophysics Centre, Aarhus University, Denmark # Rachel Street Las Cumbres Observatory, USA # Josep Manel Carrasco Universitat de Barcelona # Marco Lam Tel Aviv University, Israel # Akihiko Fukui The University of Tokyo, Japan # Mateusz Bronikowski Astronomical Observatory, University of Warsaw, Poland # Dmitry Blinov Institute of Astrophysics, FORTH, Greece # Dirk Froebrich University of Kent # Charles Galdies University of Malta # Morgan Fraser University College Dublin, Ireland # Nikolaos Mandarakas University of Crete, Physics Department, Greece # Iair Arcavi Tel Aviv University, Israel # Malhar Kendurkar Prince George Astronomical Observatory, Canada # Nami Mowlavi Department of Astronomy, University of Geneva, CH # Klaas Wiersema University of Warwick, UK # Hasan H. Esenoglu Istanbul University Observatory, University Central Campus, Beyazit, Fatih, Istanbul, Turkey # John Davies OPTICON, UK # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław, Poland # Fraser Lewis Faulkes Telescope Project & National Schools' Observatory, UK # Maja Jabłońska University of Warsaw, Poland # Szymon Kozlowski Astronomical Observatory, University of Warsaw , Poland # Katarzyna Kruszyńska Astronomical Observatory, University of Warsaw, Poland # Pawel Zielinski Astronomical Observatory, University of Warsaw, Poland # Algita Stankevičiūtė Astronomical observatory of the University of Warsaw, Poland # Gaspar Bakos Princeton University, USA # Mariusz Gromadzki Astronomical Observatory, University of Warsaw, Poland # Nariman Ismailov Shamakhi Astrophysical Observatory, Azerbeijan # Benny Trakhtenbrot Tel Aviv University, Israel # Tsvi Piran The Hebrew University , Israel # Ashish Mahabal Caltech, USA # Ilknur Gezer Warsaw University Astronomical Observatory, Poland # Gábor Marton CSFK Konkoly Observatory, Hungary # Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungary # Michel Dennefeld IAP-Paris, France # Goran Damljanovic Astronomical Observatory, Serbia # Jaroslav Merc Astronomical Institute of Charles University in Prague, Czechia # Roberto Alexander Cerviño Department of Data Science, Faculty of Computer Science, Multimedia and Telecommunications, Universitat Oberta de Catalunya # Michał Siwak Konkoly Observatory, Hungary # Nada Ihanec Astronomical Observatory, University of Warsaw, Poland # William Thuillot Paris Observatory / IMCCE, France # Ruta Urbonaviciute Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Kris Rybicki Astronomical Observatory, University of Warsaw, Poland # Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University, Lithuania # Justas Zdanavičius Astronomical Observatory of the Vilnius University, Lithuania # Etienne Bachelet Las Cumbres Observatory, USA # Przemek Mroz California Institute of Technology, USA # Zofia Kaczmarek Warsaw University Astronomical Observatory, Poland # Agnieszka Słowikowska Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland # Maria Gabriela Navarro Sapienza / MAS / UNAB, Chile/Italy # Zuzanna Kostrzewa-Rutkowska Leiden Observatory, NL # Benito Marcote Joint Institute for VLBI ERIC (JIVE), NL # Artie Hatzes Thüringer Landessternwarte Tautenburg, Germany # Nicholas Rattenbury The University of Auckland, New Zeleand # Takahiro Sumi Osaka University, Japan # Gerry Gilmore IoA Cambridge, UK # Eran Ofek Weizmann Institute of Science, Israel # Simon Hodgkin University of Cambridge, UK # Harro Verkouter Joint Institute for VLBI in Europe, NL # Marzena Sniegowska Nicolaus Copernicus Astronomical Center Polish Academy of Sciences, Poland # Maria Jose Rain Universita' degli studi di Padova, Italy # Aayush Gautam Birendra Multiple Campus, Tribhuvan University, Nepal # Timur Şahin Akdeniz University, Turkey # László Szabados Konkoly Observatory, Hungary # Andrzej Pigulski University of Wrocław, Poland # Monika Kamińska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University, Poland # Stephen Brincat Flarestar Observatory (MPC:171); AAVSO # Krzysztof Kamiński Astronomical Observatory of Adam Mickiewicz University, Poland # Prasanta Kumar Nayak Tata Institute of Fundamental Research, Mumbai, India # Sepideh Eskandarlou Kharazmi university, Iran # Michał Żejmo Instytut Astronomii im. profesora Janusza Gila, Uniwersytet Zielonogórski, Poland # Yogesh Joshi Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, India # Lydia Makrygianni Tel Aviv University, Israel # Waldemar Ogloza Mt.Suhora Observatory, Cracow Pedagogical University, Poland # Laura Ruiz-Dern Department of Data Science, Faculty of Computer Science, Multimedia and Telecommunications, Universitat Oberta de Catalunya # Areg Mickaelian Byurakan Astrophysical Observatory (BAO), Armenia # Staszek Zola Astronomical Observatory, Jagiellonian University, Poland # Roberto Figuera Jaimes San Sebastian University, USA # Milena Ratajczak Astronomical Observatory, University of Warsaw, Poland # Salim Ansari ESA - ESTEC # Mike Garrett University of Manchester, UK # Franz-Josef Hambsch Vereniging Voor Sterrenkunde (VVS), Oostmeers 122 C, 8000 Brugge, Belgium # Ryszard Szczerba Nicolaus Copernicus Astronomical Center, Poland # Karolina Bąkowska N. Copernicus University, Poland # Emma Dodd Kapteyn, University of Groningen, NL # Siegfried Vanaverbeke astrolab IRIS observatory # Elahe Khalouei Sharif university of technology, Iran # Kotryna Siskauskaite Vilnius University, Lithuania # Ágnes Kóspál Konkoly Observatory, Budapest, Hungary # Péter Ábrahám Konkoly Observatory, Hungary # Aishwarya Selvaraj University of Manchester, UK # Sunkyung Park Konkoly Observatory, Hungary # Markus Hundertmark ARI, Zentrum für Astronomie, Universität Heidelberg, Germany # Erika Pakštienė Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Vytautas Čepas Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Seppo Mattila University of Turku, Finland # Lorenzo Rimoldini University of Geneva, CH # Krzysztof Nienartowicz ESA Gaia DPCG/CU7, Geneva, CH # Laurent Eyer Universit of Geneva, CH # Berry Holl Department of Astronomy, Geneva, CH # Shri Kulkarni Caltech, USA # Malgorzata van Leeuwen Institute of Astronomy, University of Cambridge, UK # Cristina Barbarino Tel Aviv University, IL # Simon Hodgkin Institute of Astronomy, University of Cambridge, UK # Mikołaj Kałuszyński Nicolaus Copernicus Astronomical Center, Poland # Timo Prusti ESA, NL # Guy Rixon IoA Cambridge, UK # Elme Breedt IoA, University of Cambridge, UK # Gudrun Pebody IoA, University of Cambridge, UK 5cd7f6eb7e37c611d4b2dcacded190cd8ec32b79 2650 2629 2021-01-22T06:37:17Z Gsawgwikiadmin 1 wikitext text/x-wiki The requests for talks is now closed. However, if you feel you still need to register, please email Lukasz Wyrzykowski lw at astrouw.edu.pl. <!--- ''After the registration process, you will be asked to select your preferred time slot. Please select as many as possible for different days and times. Please check the [[Workshop2020:agenda|agenda page]] for more details.'' <big>'''[https://forms.gle/5teX8EfRgh4VsyP26 CLICK HERE FOR THE REGISTRATION FORM]'''</big> Please note that due to technical limitations we can only accept 100 online attendees. The WOC will consider all applications and will inform the accepted participants, who will then receive the link to the online workshop. ---> == Registered participants == # Karsten Brogaard Stellar astrophysics Centre, Aarhus University, Denmark # Rachel Street Las Cumbres Observatory, USA # Josep Manel Carrasco Universitat de Barcelona # Marco Lam Tel Aviv University, Israel # Akihiko Fukui The University of Tokyo, Japan # Mateusz Bronikowski Astronomical Observatory, University of Warsaw, Poland # Dmitry Blinov Institute of Astrophysics, FORTH, Greece # Dirk Froebrich University of Kent # Charles Galdies University of Malta # Morgan Fraser University College Dublin, Ireland # Nikolaos Mandarakas University of Crete, Physics Department, Greece # Iair Arcavi Tel Aviv University, Israel # Malhar Kendurkar Prince George Astronomical Observatory, Canada # Nami Mowlavi Department of Astronomy, University of Geneva, CH # Klaas Wiersema University of Warwick, UK # Hasan H. Esenoglu Istanbul University Observatory, University Central Campus, Beyazit, Fatih, Istanbul, Turkey # John Davies OPTICON, UK # Przemysław Mikołajczyk Astronomical Institute, University of Wrocław, Poland # Fraser Lewis Faulkes Telescope Project & National Schools' Observatory, UK # Maja Jabłońska University of Warsaw, Poland # Szymon Kozlowski Astronomical Observatory, University of Warsaw , Poland # Katarzyna Kruszyńska Astronomical Observatory, University of Warsaw, Poland # Pawel Zielinski Astronomical Observatory, University of Warsaw, Poland # Algita Stankevičiūtė Astronomical observatory of the University of Warsaw, Poland # Gaspar Bakos Princeton University, USA # Mariusz Gromadzki Astronomical Observatory, University of Warsaw, Poland # Nariman Ismailov Shamakhi Astrophysical Observatory, Azerbeijan # Benny Trakhtenbrot Tel Aviv University, Israel # Tsvi Piran The Hebrew University , Israel # Ashish Mahabal Caltech, USA # Ilknur Gezer Warsaw University Astronomical Observatory, Poland # Gábor Marton CSFK Konkoly Observatory, Hungary # Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungary # Michel Dennefeld IAP-Paris, France # Goran Damljanovic Astronomical Observatory, Serbia # Jaroslav Merc Astronomical Institute of Charles University in Prague, Czechia # Roberto Alexander Cerviño Department of Data Science, Faculty of Computer Science, Multimedia and Telecommunications, Universitat Oberta de Catalunya # Michał Siwak Konkoly Observatory, Hungary # Nada Ihanec Astronomical Observatory, University of Warsaw, Poland # William Thuillot Paris Observatory / IMCCE, France # Ruta Urbonaviciute Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Kris Rybicki Astronomical Observatory, University of Warsaw, Poland # Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University, Lithuania # Justas Zdanavičius Astronomical Observatory of the Vilnius University, Lithuania # Etienne Bachelet Las Cumbres Observatory, USA # Przemek Mroz California Institute of Technology, USA # Zofia Kaczmarek Warsaw University Astronomical Observatory, Poland # Agnieszka Słowikowska Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland # Maria Gabriela Navarro Sapienza / MAS / UNAB, Chile/Italy # Zuzanna Kostrzewa-Rutkowska Leiden Observatory, NL # Benito Marcote Joint Institute for VLBI ERIC (JIVE), NL # Artie Hatzes Thüringer Landessternwarte Tautenburg, Germany # Nicholas Rattenbury The University of Auckland, New Zeleand # Takahiro Sumi Osaka University, Japan # Gerry Gilmore IoA Cambridge, UK # Eran Ofek Weizmann Institute of Science, Israel # Simon Hodgkin University of Cambridge, UK # Harro Verkouter Joint Institute for VLBI in Europe, NL # Marzena Sniegowska Nicolaus Copernicus Astronomical Center Polish Academy of Sciences, Poland # Maria Jose Rain Universita' degli studi di Padova, Italy # Aayush Gautam Birendra Multiple Campus, Tribhuvan University, Nepal # Timur Şahin Akdeniz University, Turkey # László Szabados Konkoly Observatory, Hungary # Andrzej Pigulski University of Wrocław, Poland # Monika Kamińska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University, Poland # Stephen Brincat Flarestar Observatory (MPC:171); AAVSO # Krzysztof Kamiński Astronomical Observatory of Adam Mickiewicz University, Poland # Prasanta Kumar Nayak Tata Institute of Fundamental Research, Mumbai, India # Sepideh Eskandarlou Kharazmi university, Iran # Michał Żejmo Instytut Astronomii im. profesora Janusza Gila, Uniwersytet Zielonogórski, Poland # Yogesh Joshi Aryabhatta Research Institute of Observational Sciences (ARIES), Nainital, India # Lydia Makrygianni Tel Aviv University, Israel # Waldemar Ogloza Mt.Suhora Observatory, Cracow Pedagogical University, Poland # Laura Ruiz-Dern Department of Data Science, Faculty of Computer Science, Multimedia and Telecommunications, Universitat Oberta de Catalunya # Areg Mickaelian Byurakan Astrophysical Observatory (BAO), Armenia # Staszek Zola Astronomical Observatory, Jagiellonian University, Poland # Roberto Figuera Jaimes San Sebastian University, Chile # Milena Ratajczak Astronomical Observatory, University of Warsaw, Poland # Salim Ansari ESA - ESTEC # Mike Garrett University of Manchester, UK # Franz-Josef Hambsch Vereniging Voor Sterrenkunde (VVS), Oostmeers 122 C, 8000 Brugge, Belgium # Ryszard Szczerba Nicolaus Copernicus Astronomical Center, Poland # Karolina Bąkowska N. Copernicus University, Poland # Emma Dodd Kapteyn, University of Groningen, NL # Siegfried Vanaverbeke astrolab IRIS observatory # Elahe Khalouei Sharif university of technology, Iran # Kotryna Siskauskaite Vilnius University, Lithuania # Ágnes Kóspál Konkoly Observatory, Budapest, Hungary # Péter Ábrahám Konkoly Observatory, Hungary # Aishwarya Selvaraj University of Manchester, UK # Sunkyung Park Konkoly Observatory, Hungary # Markus Hundertmark ARI, Zentrum für Astronomie, Universität Heidelberg, Germany # Erika Pakštienė Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Vytautas Čepas Institute of Theoretical Physics and Astronomy at Vilnius University, Lithuania # Seppo Mattila University of Turku, Finland # Lorenzo Rimoldini University of Geneva, CH # Krzysztof Nienartowicz ESA Gaia DPCG/CU7, Geneva, CH # Laurent Eyer Universit of Geneva, CH # Berry Holl Department of Astronomy, Geneva, CH # Shri Kulkarni Caltech, USA # Malgorzata van Leeuwen Institute of Astronomy, University of Cambridge, UK # Cristina Barbarino Tel Aviv University, IL # Simon Hodgkin Institute of Astronomy, University of Cambridge, UK # Mikołaj Kałuszyński Nicolaus Copernicus Astronomical Center, Poland # Timo Prusti ESA, NL # Guy Rixon IoA Cambridge, UK # Elme Breedt IoA, University of Cambridge, UK # Gudrun Pebody IoA, University of Cambridge, UK 3059ead38264d01abe60782495d9715d069b871d 0 334 2608 2602 2021-01-12T17:25:48Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held for about 3h every of 5 days. The times will alternate to suit different time-zones. The programme will be composed of presentations from participants. During the registration, there will be a Doodle Poll, where you will be able to propose your best time slots for your presentation. Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool. The link to Wonder Room will be provided to the registered participants. [[File:schedulePoll.png|300px]] ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- [[File:Agenda-draft.pdf]] d88837e2fbb041f24fcfcc425d55a3346bbef142 2610 2608 2021-01-12T17:27:17Z Gsawgwikiadmin 1 wikitext text/x-wiki Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- [[File:Agenda-draft.pdf]] 10cf61199c876b0abb8c97acb4d3a0e2182d97f9 2613 2610 2021-01-13T15:34:44Z Gsawgwikiadmin 1 wikitext text/x-wiki Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] <!--- ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- ---> 1882221b3782bbd0f85677c57b426a9d0a4e72ca 2614 2613 2021-01-13T15:35:11Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. <!--- ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |---- |} ---- ---> d1302cba2b17c46e58db896bbec8e85466a61d88 2621 2614 2021-01-13T17:11:07Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 21.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 784e877473be0b483cdb1dc774db289072dce432 2628 2621 2021-01-15T09:54:11Z Zuzanna 36 /* Time table and YouTube stream */ wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- f2b40de48472c8286fd35534e59f704f28e235c3 2630 2628 2021-01-17T06:37:27Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[Media:Agenda2020.pdf]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 4b7c3f3aa00894aba30e9e8b379ffefdd75df4f7 2632 2630 2021-01-17T06:38:15Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[File:Abstracts2020.pdf]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 0b3ec8c4fc50386e325bf18490b3b84c3f8ac9b6 2634 2632 2021-01-17T06:38:58Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[File:Abstracts2020.pdf Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 0c6f1b67c9fb38cab7a5055481c71f523bf0a6f3 2635 2634 2021-01-17T06:39:04Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[File:Abstracts2020.pdf |Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 51fac80b5ddaf8a8ba91348e150cafbdfebebbf7 2636 2635 2021-01-17T06:39:16Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[File:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- d562d86244ad9deff6fd4872266c431a1d6e7efa 2637 2636 2021-01-17T06:39:32Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [File:Abstracts2020.pdf|Abstracts book] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 6c1d2ddf28747bc4c0a0e2187833084340bbe2c1 2638 2637 2021-01-17T06:39:42Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[File:Abstracts2020.pdf|Abstracts book][ </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 78d9ee0e849891aa276b0ce2784e5b341fda41ec 2639 2638 2021-01-17T06:39:50Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[File:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- d562d86244ad9deff6fd4872266c431a1d6e7efa 2640 2639 2021-01-17T06:40:26Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda (draft)] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 33fc498f871787f5966230e755441577cbf8b27f 2641 2640 2021-01-17T16:32:26Z Gsawgwikiadmin 1 wikitext text/x-wiki <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 1e27defd5bc9180d1f6363e5ceb7bde6d164f801 2642 2641 2021-01-18T10:23:25Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- f461f2931c19cf4d9dd8ff155fc3e0d0ee66457c 2643 2642 2021-01-18T10:23:40Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- a13fbf86f04b9c57365bf711e9e41734fe195825 2646 2643 2021-01-18T18:28:54Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am | |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- a328d09594b4c4a73d0ed5f8f443bfa6cb1306e0 2647 2646 2021-01-19T15:25:46Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am | |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- 70c0ae42ac4729ee49edf1cac3bb92746c42b9e3 2648 2647 2021-01-20T20:37:04Z Gsawgwikiadmin 1 /* Time table and YouTube stream */ wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am | |---- |} ---- e55f65c7c1f48bae84e73469ed361674c3434e5d 2649 2648 2021-01-21T16:00:50Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- bb15b02f53867d43eaf1879ff7becc8ff30be233 2651 2649 2021-03-02T15:36:55Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Monday 18 January 2021'''</big> |---- |15:00 |Lukasz Wyrzykowski |Welcome and technical information |0:05 |---- |15:05 |Marek Moszyński |Welcome address from the President of the Polish Space Agency |0:05 |---- |15:10 |Timo Prusti |Gaia overview |0:30 |---- |15:40 |Simon Hodgkin |Gaia Science Alerts: Status of the system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:25 |---- |16:05 |Gerry Gilmore |Gaia, OPTICON, ORP and time-domain astronomy |0:25 |---- |16:30 |John Davies |TDA in the OPTICON Radionet PILOT |0:15 |---- |16:45 |Harro Verkouter |ORP - PILOT = TOM + EVN |0:15 |---- |17:00 |Break | |0:15 |---- |17:15 |Lukasz Wyrzykowski |Introduction to the Black Hole Target Observation Manager (BHTOM) |0:15 |---- |17:30 |Maja Jabłońska |Black Hole Target Observation Manager |0:15 |---- |17:45 |Paweł Zieliński |Uploading data to BHTOM |0:15 |---- |18:00 |Przemysław Mikołajczyk |CCDPhot for automated photometric processing |0:15 |---- |18:15 |Mikołaj Kałuszyński |Webservices in scientific applications, CCDPHOTsvc |0:15 |---- |18:30 |Rachel Street |Software tools to enhance alert-based science |0:05 |---- | | | | |---- |colspan="4"|<big>'''Tuesday 19 January 2021'''</big> |---- |10:00 |Pawel Zielinski |Spectroscopic classification of Gaia microlensing event candidates |0:15 |---- |10:15 |Gábor Marton |Classification of Gaia Alerts with machine learning algorithms |0:15 |---- |10:30 |Ilknur Gezer |Photometric classification of Gaia microlensing event candidates with machine learning methods |0:15 |---- |10:45 |Roberto Alexander Cerviño |Automatic classification of Gaia Photometric Alerts using spectra data through Machine Learning and Deep Learning. |0:15 |---- |11:00 |Nicholas Rattenbury |New Zealand Time Critical Astrophysics |0:15 |---- |11:15 |Takahiro Sumi |PRIME |0:15 |---- |11:30 |Maria Gabriela Navarro |VVV Microlensing events in the Galactic bulge |0:15 |---- |11:45 |Akihiko Fukui |Photometry of Gaia Microlensing Events from Tomo-e Gozen Survey |0:05 |---- |11:50 |Break | |0:25 |---- |12:15 |Eran Ofek |The Large Array Survey Telescope and time delay estimation |0:30 |---- |12:45 |Mariusz Gromadzki |OGLE-IV Transient Search |0:15 |---- |13:00 |Zuzanna Kostrzewa-Rutkowska |Electromagnetic counterparts of gravitational wave sources with Gaia |0:15 |---- |13:15 |Hasan H. Esenoglu |Spectroscopy and Photometry of Gaia20eld (Nova Cas 2020) |0:15 |---- |13:30 |Krzysztof Kaminski |Science with RBT/PST2 and PST3 telescopes. |0:15 |---- |13:45 |Zsofia Nagy |Dipper-like variability of the Gaia alerted young star V555 Ori |0:15 |---- | | | | |---- |18:00 |WonderMe platform |Hands-on in data uploading in BHTOM led by Pawel Zielinski | |---- | | | | |---- |colspan="4"|<big>'''Wednesday 20 January 2021'''</big> |---- | | | | |---- |15:00 |Zoom |Hands-on in data uploading in BHTOM led by Pawel Zielinski (repeated) | |---- | | | | |---- |18:00 |Nami Mowlavi |Overview of variable objects processing within the Gaia consortium |0:25 |---- |18:25 |William Thuillot |Gaia follow-up of the uncatalogued Solar System Objects |0:15 |---- |18:40 |Dirk Froebrich |Gaia Alert Follow up with the HOYS Citizen Science project |0:15 |---- |18:55 |Malhar Kendurkar |Data Analysis and Search for Astronomical Transients (AT's) |0:05 |---- |19:00 |Katarzyna Kruszyńska |Microlensing Highlights in Gaia Science Alerts |0:15 |---- |19:15 |Kris Rybicki |Update on Gaia19bld event |0:15 |---- |19:30 |Break | |0:15 |---- |19:45 |Zofia Kaczmarek |Lensing events with parallax in Gaia Alerts |0:15 |---- |20:00 |Marius Maskoliunas |Preliminary results for the microlensing event Gaia19dke |0:15 |---- |20:15 |Ashish Mahabal |ZTF, ML, and Variability |0:15 |---- |20:30 |Przemek Mroz |All-sky searches for gravitational microlensing events with data from the Zwicky Transient Facility |0:15 |---- |20:45 |Etienne Bachelet |The OMEGA Key Project : detection of cold planets and stellar remnants in the entire Milky Way |0:15 |---- | | | | |---- | | | | |---- |colspan="4"|<big>'''Thursday 21 January 2021'''</big> |---- |10:00 |Iair Arcavi |TDEs overview |0:15 |---- |10:15 |Nada Ihanec |Bowen Fluorescence Flares - new class of nuclear transients |0:05 |---- |10:20 |Szymon Kozlowski |Quasar Variability in Gaia: Simulation Perspective |0:15 |---- |10:35 |Morgan Fraser |Supernovae and Gaia |0:15 |---- |10:50 |Mateusz Bronikowski |Overluminous transients in Gaia Alerts using photometric redshift |0:05 |---- |10:55 |Benny Trakhtenbrot |Resolving the Mystery of Changing Look AGN with Responsive Follow-up Observations |0:15 |---- |11:10 |Break | |0:30 |---- |11:40 |Tsvi Piran |TDEs in AGNs |0:15 |---- |11:55 |Nikolaos Mandarakas |Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique |0:15 |---- |12:10 |Benito Marcote |Discovering radio transients from Gaia Alerts |0:15 |---- |12:25 |Dmitry Blinov |On the need of optical polarimetry follow up of flaring AGN in Gaia alerts |0:05 |---- |12:30 |Jaroslav Merc |Gaia18aen: First symbiotic star discovered by Gaia |0:15 |---- |12:45 |Michał Siwak |In search for new eruptive young stars among Gaia Alerts |0:15 |---- |13:00 |Artie Hatzes |The Alfred Jensch 2m Telescope and its Use for Targets of Opportunity |0:15 |---- |13:15 |Klaas Wiersema |A snapshot survey of polarised light in optical transients |0:15 |---- | | | | |---- |colspan="4"|<big>'''Friday 22 January 2021'''</big> |---- |15:05 |Gaspar Bakos |Monitoring the sky with HATPI |0:15 |---- |15:20 |Josep Manel Carrasco |Science alerts from the Joan Oró telescope |0:05 |---- |15:25 |Marco Lam |First glimpse of the new LT/SPRAT automated pipeline with ASPIRED |0:05 |---- |15:30 |Stephen Brincat & Charles Galdies |Time-series photometry from Flarestar Observatory – Malta |0:15 |---- |15:45 |Michel Dennefeld |Follow-up of some Gaia Alerts |0:15 |---- |16:00 |Break | |0:20 |---- |16:20 |Goran Damljanovic |Gaia Alerts and the Serbian-Bulgarian mini-network telescopes during 2020 |0:15 |---- |16:35 |Justas Zdanavičius |Gaia alert observations and reductions in Lithuania |0:15 |---- |16:50 |Ruta Urbonaviciute |Search for variable stars in the northern sky |0:05 |---- |16:55 |Algita Stankevičiūtė |Future of detecting Black Holes with ground-based telescopes |0:05 |---- |17:00 |Karsten Brogaard |Educational telescope at Mt. Kent |0:05 |---- |17:05 |Fraser Lewis |Linking Education and Research Using Robotic Telescopes |0:15 |---- |17:20 |Agnieszka Słowikowska |Orbital and physical parameters distributions of exoplanets in the light of Gaia DR2 catalogue |0:05 |---- |17:25 |Summary | |0:15 |---- | | | | |---- |17:40 |'''Social meeting on WonderMe''' | | |} e14bf4bed8cafba4f0b0d598c6f17a4f679768a8 2652 2651 2021-03-02T15:54:38Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Monday 18 January 2021'''</big> |---- |15:00 |Lukasz Wyrzykowski |Welcome and technical information |0:05 |---- |15:05 |Marek Moszyński |Welcome address from the President of the Polish Space Agency |0:05 |---- |15:10 |Timo Prusti |Gaia overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:30 |---- |15:40 |Simon Hodgkin |Gaia Science Alerts: Status of the system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:25 |---- |16:05 |Gerry Gilmore |Gaia, OPTICON, ORP and time-domain astronomy |0:25 |---- |16:30 |John Davies |TDA in the OPTICON Radionet PILOT |0:15 |---- |16:45 |Harro Verkouter |ORP - PILOT = TOM + EVN |0:15 |---- |17:00 |Break | |0:15 |---- |17:15 |Lukasz Wyrzykowski |Introduction to the Black Hole Target Observation Manager (BHTOM) |0:15 |---- |17:30 |Maja Jabłońska |Black Hole Target Observation Manager |0:15 |---- |17:45 |Paweł Zieliński |Uploading data to BHTOM |0:15 |---- |18:00 |Przemysław Mikołajczyk |CCDPhot for automated photometric processing |0:15 |---- |18:15 |Mikołaj Kałuszyński |Webservices in scientific applications, CCDPHOTsvc |0:15 |---- |18:30 |Rachel Street |Software tools to enhance alert-based science |0:05 |---- | | | | |---- |colspan="4"|<big>'''Tuesday 19 January 2021'''</big> |---- |10:00 |Pawel Zielinski |Spectroscopic classification of Gaia microlensing event candidates |0:15 |---- |10:15 |Gábor Marton |Classification of Gaia Alerts with machine learning algorithms |0:15 |---- |10:30 |Ilknur Gezer |Photometric classification of Gaia microlensing event candidates with machine learning methods |0:15 |---- |10:45 |Roberto Alexander Cerviño |Automatic classification of Gaia Photometric Alerts using spectra data through Machine Learning and Deep Learning. |0:15 |---- |11:00 |Nicholas Rattenbury |New Zealand Time Critical Astrophysics |0:15 |---- |11:15 |Takahiro Sumi |PRIME |0:15 |---- |11:30 |Maria Gabriela Navarro |VVV Microlensing events in the Galactic bulge |0:15 |---- |11:45 |Akihiko Fukui |Photometry of Gaia Microlensing Events from Tomo-e Gozen Survey |0:05 |---- |11:50 |Break | |0:25 |---- |12:15 |Eran Ofek |The Large Array Survey Telescope and time delay estimation |0:30 |---- |12:45 |Mariusz Gromadzki |OGLE-IV Transient Search |0:15 |---- |13:00 |Zuzanna Kostrzewa-Rutkowska |Electromagnetic counterparts of gravitational wave sources with Gaia |0:15 |---- |13:15 |Hasan H. Esenoglu |Spectroscopy and Photometry of Gaia20eld (Nova Cas 2020) |0:15 |---- |13:30 |Krzysztof Kaminski |Science with RBT/PST2 and PST3 telescopes. |0:15 |---- |13:45 |Zsofia Nagy |Dipper-like variability of the Gaia alerted young star V555 Ori |0:15 |---- | | | | |---- |18:00 |WonderMe platform |Hands-on in data uploading in BHTOM led by Pawel Zielinski | |---- | | | | |---- |colspan="4"|<big>'''Wednesday 20 January 2021'''</big> |---- | | | | |---- |15:00 |Zoom |Hands-on in data uploading in BHTOM led by Pawel Zielinski (repeated) | |---- | | | | |---- |18:00 |Nami Mowlavi |Overview of variable objects processing within the Gaia consortium |0:25 |---- |18:25 |William Thuillot |Gaia follow-up of the uncatalogued Solar System Objects |0:15 |---- |18:40 |Dirk Froebrich |Gaia Alert Follow up with the HOYS Citizen Science project |0:15 |---- |18:55 |Malhar Kendurkar |Data Analysis and Search for Astronomical Transients (AT's) |0:05 |---- |19:00 |Katarzyna Kruszyńska |Microlensing Highlights in Gaia Science Alerts |0:15 |---- |19:15 |Kris Rybicki |Update on Gaia19bld event |0:15 |---- |19:30 |Break | |0:15 |---- |19:45 |Zofia Kaczmarek |Lensing events with parallax in Gaia Alerts |0:15 |---- |20:00 |Marius Maskoliunas |Preliminary results for the microlensing event Gaia19dke |0:15 |---- |20:15 |Ashish Mahabal |ZTF, ML, and Variability |0:15 |---- |20:30 |Przemek Mroz |All-sky searches for gravitational microlensing events with data from the Zwicky Transient Facility |0:15 |---- |20:45 |Etienne Bachelet |The OMEGA Key Project : detection of cold planets and stellar remnants in the entire Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/EtienneBachelet.pdf PDF] |0:15 |---- | | | | |---- | | | | |---- |colspan="4"|<big>'''Thursday 21 January 2021'''</big> |---- |10:00 |Iair Arcavi |TDEs overview |0:15 |---- |10:15 |Nada Ihanec |Bowen Fluorescence Flares - new class of nuclear transients |0:05 |---- |10:20 |Szymon Kozlowski |Quasar Variability in Gaia: Simulation Perspective |0:15 |---- |10:35 |Morgan Fraser |Supernovae and Gaia |0:15 |---- |10:50 |Mateusz Bronikowski |Overluminous transients in Gaia Alerts using photometric redshift |0:05 |---- |10:55 |Benny Trakhtenbrot |Resolving the Mystery of Changing Look AGN with Responsive Follow-up Observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/BennyTrakhtenbrot.pdf PDF] |0:15 |---- |11:10 |Break | |0:30 |---- |11:40 |Tsvi Piran |TDEs in AGNs |0:15 |---- |11:55 |Nikolaos Mandarakas |Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique |0:15 |---- |12:10 |Benito Marcote |Discovering radio transients from Gaia Alerts |0:15 |---- |12:25 |Dmitry Blinov |On the need of optical polarimetry follow up of flaring AGN in Gaia alerts |0:05 |---- |12:30 |Jaroslav Merc |Gaia18aen: First symbiotic star discovered by Gaia |0:15 |---- |12:45 |Michał Siwak |In search for new eruptive young stars among Gaia Alerts |0:15 |---- |13:00 |Artie Hatzes |The Alfred Jensch 2m Telescope and its Use for Targets of Opportunity |0:15 |---- |13:15 |Klaas Wiersema |A snapshot survey of polarised light in optical transients |0:15 |---- | | | | |---- |colspan="4"|<big>'''Friday 22 January 2021'''</big> |---- |15:05 |Gaspar Bakos |Monitoring the sky with HATPI |0:15 |---- |15:20 |Josep Manel Carrasco |Science alerts from the Joan Oró telescope |0:05 |---- |15:25 |Marco Lam |First glimpse of the new LT/SPRAT automated pipeline with ASPIRED |0:05 |---- |15:30 |Stephen Brincat & Charles Galdies |Time-series photometry from Flarestar Observatory – Malta |0:15 |---- |15:45 |Michel Dennefeld |Follow-up of some Gaia Alerts |0:15 |---- |16:00 |Break | |0:20 |---- |16:20 |Goran Damljanovic |Gaia Alerts and the Serbian-Bulgarian mini-network telescopes during 2020 |0:15 |---- |16:35 |Justas Zdanavičius |Gaia alert observations and reductions in Lithuania |0:15 |---- |16:50 |Ruta Urbonaviciute |Search for variable stars in the northern sky |0:05 |---- |16:55 |Algita Stankevičiūtė |Future of detecting Black Holes with ground-based telescopes |0:05 |---- |17:00 |Karsten Brogaard |Educational telescope at Mt. Kent |0:05 |---- |17:05 |Fraser Lewis |Linking Education and Research Using Robotic Telescopes |0:15 |---- |17:20 |Agnieszka Słowikowska |Orbital and physical parameters distributions of exoplanets in the light of Gaia DR2 catalogue |0:05 |---- |17:25 |Summary | |0:15 |---- | | | | |---- |17:40 |'''Social meeting on WonderMe''' | | |} 7d719064e37aea238c5f8c468127622fa8d50516 2653 2652 2021-03-02T16:08:16Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Monday 18 January 2021'''</big> |---- |15:00 |Lukasz Wyrzykowski |Welcome and technical information |0:05 |---- |15:05 |Marek Moszyński |Welcome address from the President of the Polish Space Agency |0:05 |---- |15:10 |Timo Prusti |Gaia overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:30 |---- |15:40 |Simon Hodgkin |Gaia Science Alerts: Status of the system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:25 |---- |16:05 |Gerry Gilmore |Gaia, OPTICON, ORP and time-domain astronomy |0:25 |---- |16:30 |John Davies |TDA in the OPTICON Radionet PILOT |0:15 |---- |16:45 |Harro Verkouter |ORP - PILOT = TOM + EVN |0:15 |---- |17:00 |Break | |0:15 |---- |17:15 |Lukasz Wyrzykowski |Introduction to the Black Hole Target Observation Manager (BHTOM) |0:15 |---- |17:30 |Maja Jabłońska |Black Hole Target Observation Manager |0:15 |---- |17:45 |Paweł Zieliński |Uploading data to BHTOM [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski.pdf PDF] |0:15 |---- |18:00 |Przemysław Mikołajczyk |CCDPhot for automated photometric processing |0:15 |---- |18:15 |Mikołaj Kałuszyński |Webservices in scientific applications, CCDPHOTsvc |0:15 |---- |18:30 |Rachel Street |Software tools to enhance alert-based science [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RachelStreet.pdf PDF] |0:05 |---- | | | | |---- |colspan="4"|<big>'''Tuesday 19 January 2021'''</big> |---- |10:00 |Pawel Zielinski |Spectroscopic classification of Gaia microlensing event candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-spec.pdf PDF] |0:15 |---- |10:15 |Gábor Marton |Classification of Gaia Alerts with machine learning algorithms |0:15 |---- |10:30 |Ilknur Gezer |Photometric classification of Gaia microlensing event candidates with machine learning methods |0:15 |---- |10:45 |Roberto Alexander Cerviño |Automatic classification of Gaia Photometric Alerts using spectra data through Machine Learning and Deep Learning. |0:15 |---- |11:00 |Nicholas Rattenbury |New Zealand Time Critical Astrophysics |0:15 |---- |11:15 |Takahiro Sumi |PRIME |0:15 |---- |11:30 |Maria Gabriela Navarro |VVV Microlensing events in the Galactic bulge |0:15 |---- |11:45 |Akihiko Fukui |Photometry of Gaia Microlensing Events from Tomo-e Gozen Survey |0:05 |---- |11:50 |Break | |0:25 |---- |12:15 |Eran Ofek |The Large Array Survey Telescope and time delay estimation |0:30 |---- |12:45 |Mariusz Gromadzki |OGLE-IV Transient Search |0:15 |---- |13:00 |Zuzanna Kostrzewa-Rutkowska |Electromagnetic counterparts of gravitational wave sources with Gaia |0:15 |---- |13:15 |Hasan H. Esenoglu |Spectroscopy and Photometry of Gaia20eld (Nova Cas 2020) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/HasanEsenoglu.pdf PDF] |0:15 |---- |13:30 |Krzysztof Kaminski |Science with RBT/PST2 and PST3 telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KrzysztofKaminski.pdf PDF] |0:15 |---- |13:45 |Zsofia Nagy |Dipper-like variability of the Gaia alerted young star V555 Ori |0:15 |---- | | | | |---- |18:00 |WonderMe platform |Hands-on in data uploading in BHTOM led by Pawel Zielinski [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-handson.pdf PDF] | |---- | | | | |---- |colspan="4"|<big>'''Wednesday 20 January 2021'''</big> |---- | | | | |---- |15:00 |Zoom |Hands-on in data uploading in BHTOM led by Pawel Zielinski (repeated) | |---- | | | | |---- |18:00 |Nami Mowlavi |Overview of variable objects processing within the Gaia consortium [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NamiMowlavi.pdf PDF] |0:25 |---- |18:25 |William Thuillot |Gaia follow-up of the uncatalogued Solar System Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/WilliamThuillot.pdf PDF] |0:15 |---- |18:40 |Dirk Froebrich |Gaia Alert Follow up with the HOYS Citizen Science project |0:15 |---- |18:55 |Malhar Kendurkar |Data Analysis and Search for Astronomical Transients (AT's) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MalharKendurkar.pdf PDF] |0:05 |---- |19:00 |Katarzyna Kruszyńska |Microlensing Highlights in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KatarzynaKruszynska.pdf PDF |0:15 |---- |19:15 |Kris Rybicki |Update on Gaia19bld event |0:15 |---- |19:30 |Break | |0:15 |---- |19:45 |Zofia Kaczmarek |Lensing events with parallax in Gaia Alerts |0:15 |---- |20:00 |Marius Maskoliunas |Preliminary results for the microlensing event Gaia19dke [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MariusMaskoliunas.pdf PDF] |0:15 |---- |20:15 |Ashish Mahabal |ZTF, ML, and Variability |0:15 |---- |20:30 |Przemek Mroz |All-sky searches for gravitational microlensing events with data from the Zwicky Transient Facility |0:15 |---- |20:45 |Etienne Bachelet |The OMEGA Key Project : detection of cold planets and stellar remnants in the entire Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/EtienneBachelet.pdf PDF] |0:15 |---- | | | | |---- | | | | |---- |colspan="4"|<big>'''Thursday 21 January 2021'''</big> |---- |10:00 |Iair Arcavi |TDEs overview |0:15 |---- |10:15 |Nada Ihanec |Bowen Fluorescence Flares - new class of nuclear transients |0:05 |---- |10:20 |Szymon Kozlowski |Quasar Variability in Gaia: Simulation Perspective |0:15 |---- |10:35 |Morgan Fraser |Supernovae and Gaia |0:15 |---- |10:50 |Mateusz Bronikowski |Overluminous transients in Gaia Alerts using photometric redshift |0:05 |---- |10:55 |Benny Trakhtenbrot |Resolving the Mystery of Changing Look AGN with Responsive Follow-up Observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/BennyTrakhtenbrot.pdf PDF] |0:15 |---- |11:10 |Break | |0:30 |---- |11:40 |Tsvi Piran |TDEs in AGNs |0:15 |---- |11:55 |Nikolaos Mandarakas |Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NikosMandarakas.pdf PDF] |0:15 |---- |12:10 |Benito Marcote |Discovering radio transients from Gaia Alerts |0:15 |---- |12:25 |Dmitry Blinov |On the need of optical polarimetry follow up of flaring AGN in Gaia alerts |0:05 |---- |12:30 |Jaroslav Merc |Gaia18aen: First symbiotic star discovered by Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JaroslavMerc.pdf PDF] |0:15 |---- |12:45 |Michał Siwak |In search for new eruptive young stars among Gaia Alerts |0:15 |---- |13:00 |Artie Hatzes |The Alfred Jensch 2m Telescope and its Use for Targets of Opportunity |0:15 |---- |13:15 |Klaas Wiersema |A snapshot survey of polarised light in optical transients |0:15 |---- | | | | |---- |colspan="4"|<big>'''Friday 22 January 2021'''</big> |---- |15:05 |Gaspar Bakos |Monitoring the sky with HATPI |0:15 |---- |15:20 |Josep Manel Carrasco |Science alerts from the Joan Oró telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JosepManelCarrasco.pdf PDF] |0:05 |---- |15:25 |Marco Lam |First glimpse of the new LT/SPRAT automated pipeline with ASPIRED [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MarcoLam.pdf PDF] |0:05 |---- |15:30 |Stephen Brincat & Charles Galdies |Time-series photometry from Flarestar Observatory – Malta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/StephenBrincat.pdf PDF] |0:15 |---- |15:45 |Michel Dennefeld |Follow-up of some Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MichelDennefeld.pdf PDF] |0:15 |---- |16:00 |Break | |0:20 |---- |16:20 |Goran Damljanovic |Gaia Alerts and the Serbian-Bulgarian mini-network telescopes during 2020 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/GoranDamljanovic.pdf PDF] |0:15 |---- |16:35 |Justas Zdanavičius |Gaia alert observations and reductions in Lithuania |0:15 |---- |16:50 |Ruta Urbonaviciute |Search for variable stars in the northern sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RutaUrbonaviciute.pdf PDF] |0:05 |---- |16:55 |Algita Stankevičiūtė |Future of detecting Black Holes with ground-based telescopes |0:05 |---- |17:00 |Karsten Brogaard |Educational telescope at Mt. Kent |0:05 |---- |17:05 |Fraser Lewis |Linking Education and Research Using Robotic Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/FraserLewis.pdf PDF] |0:15 |---- |17:20 |Agnieszka Słowikowska |Orbital and physical parameters distributions of exoplanets in the light of Gaia DR2 catalogue |0:05 |---- | | Nariman Ismailov | not presented [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NarimanIsmailov.pdf PDF] | |---- |17:25 |Summary | |0:15 |---- | | | | |---- |17:40 |'''Social meeting on WonderMe''' | | |} ade7b4db8defab413d69e354f55b0a2e34be5220 2654 2653 2021-03-02T16:08:59Z Gsawgwikiadmin 1 /* Workshop Agenda */ wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- == Agenda and slides == ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Monday 18 January 2021'''</big> |---- |15:00 |Lukasz Wyrzykowski |Welcome and technical information |0:05 |---- |15:05 |Marek Moszyński |Welcome address from the President of the Polish Space Agency |0:05 |---- |15:10 |Timo Prusti |Gaia overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:30 |---- |15:40 |Simon Hodgkin |Gaia Science Alerts: Status of the system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:25 |---- |16:05 |Gerry Gilmore |Gaia, OPTICON, ORP and time-domain astronomy |0:25 |---- |16:30 |John Davies |TDA in the OPTICON Radionet PILOT |0:15 |---- |16:45 |Harro Verkouter |ORP - PILOT = TOM + EVN |0:15 |---- |17:00 |Break | |0:15 |---- |17:15 |Lukasz Wyrzykowski |Introduction to the Black Hole Target Observation Manager (BHTOM) |0:15 |---- |17:30 |Maja Jabłońska |Black Hole Target Observation Manager |0:15 |---- |17:45 |Paweł Zieliński |Uploading data to BHTOM [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski.pdf PDF] |0:15 |---- |18:00 |Przemysław Mikołajczyk |CCDPhot for automated photometric processing |0:15 |---- |18:15 |Mikołaj Kałuszyński |Webservices in scientific applications, CCDPHOTsvc |0:15 |---- |18:30 |Rachel Street |Software tools to enhance alert-based science [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RachelStreet.pdf PDF] |0:05 |---- | | | | |---- |colspan="4"|<big>'''Tuesday 19 January 2021'''</big> |---- |10:00 |Pawel Zielinski |Spectroscopic classification of Gaia microlensing event candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-spec.pdf PDF] |0:15 |---- |10:15 |Gábor Marton |Classification of Gaia Alerts with machine learning algorithms |0:15 |---- |10:30 |Ilknur Gezer |Photometric classification of Gaia microlensing event candidates with machine learning methods |0:15 |---- |10:45 |Roberto Alexander Cerviño |Automatic classification of Gaia Photometric Alerts using spectra data through Machine Learning and Deep Learning. |0:15 |---- |11:00 |Nicholas Rattenbury |New Zealand Time Critical Astrophysics |0:15 |---- |11:15 |Takahiro Sumi |PRIME |0:15 |---- |11:30 |Maria Gabriela Navarro |VVV Microlensing events in the Galactic bulge |0:15 |---- |11:45 |Akihiko Fukui |Photometry of Gaia Microlensing Events from Tomo-e Gozen Survey |0:05 |---- |11:50 |Break | |0:25 |---- |12:15 |Eran Ofek |The Large Array Survey Telescope and time delay estimation |0:30 |---- |12:45 |Mariusz Gromadzki |OGLE-IV Transient Search |0:15 |---- |13:00 |Zuzanna Kostrzewa-Rutkowska |Electromagnetic counterparts of gravitational wave sources with Gaia |0:15 |---- |13:15 |Hasan H. Esenoglu |Spectroscopy and Photometry of Gaia20eld (Nova Cas 2020) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/HasanEsenoglu.pdf PDF] |0:15 |---- |13:30 |Krzysztof Kaminski |Science with RBT/PST2 and PST3 telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KrzysztofKaminski.pdf PDF] |0:15 |---- |13:45 |Zsofia Nagy |Dipper-like variability of the Gaia alerted young star V555 Ori |0:15 |---- | | | | |---- |18:00 |WonderMe platform |Hands-on in data uploading in BHTOM led by Pawel Zielinski [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-handson.pdf PDF] | |---- | | | | |---- |colspan="4"|<big>'''Wednesday 20 January 2021'''</big> |---- | | | | |---- |15:00 |Zoom |Hands-on in data uploading in BHTOM led by Pawel Zielinski (repeated) | |---- | | | | |---- |18:00 |Nami Mowlavi |Overview of variable objects processing within the Gaia consortium [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NamiMowlavi.pdf PDF] |0:25 |---- |18:25 |William Thuillot |Gaia follow-up of the uncatalogued Solar System Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/WilliamThuillot.pdf PDF] |0:15 |---- |18:40 |Dirk Froebrich |Gaia Alert Follow up with the HOYS Citizen Science project |0:15 |---- |18:55 |Malhar Kendurkar |Data Analysis and Search for Astronomical Transients (AT's) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MalharKendurkar.pdf PDF] |0:05 |---- |19:00 |Katarzyna Kruszyńska |Microlensing Highlights in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KatarzynaKruszynska.pdf PDF] |0:15 |---- |19:15 |Kris Rybicki |Update on Gaia19bld event |0:15 |---- |19:30 |Break | |0:15 |---- |19:45 |Zofia Kaczmarek |Lensing events with parallax in Gaia Alerts |0:15 |---- |20:00 |Marius Maskoliunas |Preliminary results for the microlensing event Gaia19dke [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MariusMaskoliunas.pdf PDF] |0:15 |---- |20:15 |Ashish Mahabal |ZTF, ML, and Variability |0:15 |---- |20:30 |Przemek Mroz |All-sky searches for gravitational microlensing events with data from the Zwicky Transient Facility |0:15 |---- |20:45 |Etienne Bachelet |The OMEGA Key Project : detection of cold planets and stellar remnants in the entire Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/EtienneBachelet.pdf PDF] |0:15 |---- | | | | |---- | | | | |---- |colspan="4"|<big>'''Thursday 21 January 2021'''</big> |---- |10:00 |Iair Arcavi |TDEs overview |0:15 |---- |10:15 |Nada Ihanec |Bowen Fluorescence Flares - new class of nuclear transients |0:05 |---- |10:20 |Szymon Kozlowski |Quasar Variability in Gaia: Simulation Perspective |0:15 |---- |10:35 |Morgan Fraser |Supernovae and Gaia |0:15 |---- |10:50 |Mateusz Bronikowski |Overluminous transients in Gaia Alerts using photometric redshift |0:05 |---- |10:55 |Benny Trakhtenbrot |Resolving the Mystery of Changing Look AGN with Responsive Follow-up Observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/BennyTrakhtenbrot.pdf PDF] |0:15 |---- |11:10 |Break | |0:30 |---- |11:40 |Tsvi Piran |TDEs in AGNs |0:15 |---- |11:55 |Nikolaos Mandarakas |Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NikosMandarakas.pdf PDF] |0:15 |---- |12:10 |Benito Marcote |Discovering radio transients from Gaia Alerts |0:15 |---- |12:25 |Dmitry Blinov |On the need of optical polarimetry follow up of flaring AGN in Gaia alerts |0:05 |---- |12:30 |Jaroslav Merc |Gaia18aen: First symbiotic star discovered by Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JaroslavMerc.pdf PDF] |0:15 |---- |12:45 |Michał Siwak |In search for new eruptive young stars among Gaia Alerts |0:15 |---- |13:00 |Artie Hatzes |The Alfred Jensch 2m Telescope and its Use for Targets of Opportunity |0:15 |---- |13:15 |Klaas Wiersema |A snapshot survey of polarised light in optical transients |0:15 |---- | | | | |---- |colspan="4"|<big>'''Friday 22 January 2021'''</big> |---- |15:05 |Gaspar Bakos |Monitoring the sky with HATPI |0:15 |---- |15:20 |Josep Manel Carrasco |Science alerts from the Joan Oró telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JosepManelCarrasco.pdf PDF] |0:05 |---- |15:25 |Marco Lam |First glimpse of the new LT/SPRAT automated pipeline with ASPIRED [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MarcoLam.pdf PDF] |0:05 |---- |15:30 |Stephen Brincat & Charles Galdies |Time-series photometry from Flarestar Observatory – Malta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/StephenBrincat.pdf PDF] |0:15 |---- |15:45 |Michel Dennefeld |Follow-up of some Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MichelDennefeld.pdf PDF] |0:15 |---- |16:00 |Break | |0:20 |---- |16:20 |Goran Damljanovic |Gaia Alerts and the Serbian-Bulgarian mini-network telescopes during 2020 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/GoranDamljanovic.pdf PDF] |0:15 |---- |16:35 |Justas Zdanavičius |Gaia alert observations and reductions in Lithuania |0:15 |---- |16:50 |Ruta Urbonaviciute |Search for variable stars in the northern sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RutaUrbonaviciute.pdf PDF] |0:05 |---- |16:55 |Algita Stankevičiūtė |Future of detecting Black Holes with ground-based telescopes |0:05 |---- |17:00 |Karsten Brogaard |Educational telescope at Mt. Kent |0:05 |---- |17:05 |Fraser Lewis |Linking Education and Research Using Robotic Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/FraserLewis.pdf PDF] |0:15 |---- |17:20 |Agnieszka Słowikowska |Orbital and physical parameters distributions of exoplanets in the light of Gaia DR2 catalogue |0:05 |---- | | Nariman Ismailov | not presented [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NarimanIsmailov.pdf PDF] | |---- |17:25 |Summary | |0:15 |---- | | | | |---- |17:40 |'''Social meeting on WonderMe''' | | |} d426917164fe5d09b8b80f6e96ed539ea3d78ffb 2655 2654 2021-03-04T05:39:26Z Gsawgwikiadmin 1 /* Agenda and slides */ wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- == Agenda and slides == ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Monday 18 January 2021'''</big> |---- |15:00 |Lukasz Wyrzykowski |Welcome and technical information |0:05 |---- |15:05 |Marek Moszyński |Welcome address from the President of the Polish Space Agency |0:05 |---- |15:10 |Timo Prusti |Gaia overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:30 |---- |15:40 |Simon Hodgkin |Gaia Science Alerts: Status of the system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:25 |---- |16:05 |Gerry Gilmore |Gaia, OPTICON, ORP and time-domain astronomy |0:25 |---- |16:30 |John Davies |TDA in the OPTICON Radionet PILOT |0:15 |---- |16:45 |Harro Verkouter |ORP - PILOT = TOM + EVN |0:15 |---- |17:00 |Break | |0:15 |---- |17:15 |Lukasz Wyrzykowski |Introduction to the Black Hole Target Observation Manager (BHTOM) |0:15 |---- |17:30 |Maja Jabłońska |Black Hole Target Observation Manager |0:15 |---- |17:45 |Paweł Zieliński |Uploading data to BHTOM [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski.pdf PDF] |0:15 |---- |18:00 |Przemysław Mikołajczyk |CCDPhot for automated photometric processing |0:15 |---- |18:15 |Mikołaj Kałuszyński |Webservices in scientific applications, CCDPHOTsvc |0:15 |---- |18:30 |Rachel Street |Software tools to enhance alert-based science [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RachelStreet.pdf PDF] |0:05 |---- | | | | |---- |colspan="4"|<big>'''Tuesday 19 January 2021'''</big> |---- |10:00 |Pawel Zielinski |Spectroscopic classification of Gaia microlensing event candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-spec.pdf PDF] |0:15 |---- |10:15 |Gábor Marton |Classification of Gaia Alerts with machine learning algorithms |0:15 |---- |10:30 |Ilknur Gezer |Photometric classification of Gaia microlensing event candidates with machine learning methods |0:15 |---- |10:45 |Roberto Alexander Cerviño |Automatic classification of Gaia Photometric Alerts using spectra data through Machine Learning and Deep Learning. |0:15 |---- |11:00 |Nicholas Rattenbury |New Zealand Time Critical Astrophysics |0:15 |---- |11:15 |Takahiro Sumi |PRIME |0:15 |---- |11:30 |Maria Gabriela Navarro |VVV Microlensing events in the Galactic bulge |0:15 |---- |11:45 |Akihiko Fukui |Photometry of Gaia Microlensing Events from Tomo-e Gozen Survey |0:05 |---- |11:50 |Break | |0:25 |---- |12:15 |Eran Ofek |The Large Array Survey Telescope and time delay estimation |0:30 |---- |12:45 |Mariusz Gromadzki |OGLE-IV Transient Search |0:15 |---- |13:00 |Zuzanna Kostrzewa-Rutkowska |Electromagnetic counterparts of gravitational wave sources with Gaia |0:15 |---- |13:15 |Hasan H. Esenoglu |Spectroscopy and Photometry of Gaia20eld (Nova Cas 2020) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/HasanEsenoglu.pdf PDF] |0:15 |---- |13:30 |Krzysztof Kaminski |Science with RBT/PST2 and PST3 telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KrzysztofKaminski.pdf PDF] |0:15 |---- |13:45 |Zsofia Nagy |Dipper-like variability of the Gaia alerted young star V555 Ori |0:15 |---- | | | | |---- |18:00 |WonderMe platform |Hands-on in data uploading in BHTOM led by Pawel Zielinski [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-handson.pdf PDF] | |---- | | | | |---- |colspan="4"|<big>'''Wednesday 20 January 2021'''</big> |---- | | | | |---- |15:00 |Zoom |Hands-on in data uploading in BHTOM led by Pawel Zielinski (repeated) | |---- | | | | |---- |18:00 |Nami Mowlavi |Overview of variable objects processing within the Gaia consortium [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NamiMowlavi.pdf PDF] |0:25 |---- |18:25 |William Thuillot |Gaia follow-up of the uncatalogued Solar System Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/WilliamThuillot.pdf PDF] |0:15 |---- |18:40 |Dirk Froebrich |Gaia Alert Follow up with the HOYS Citizen Science project |0:15 |---- |18:55 |Malhar Kendurkar |Data Analysis and Search for Astronomical Transients (AT's) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MalharKendurkar.pdf PDF] |0:05 |---- |19:00 |Katarzyna Kruszyńska |Microlensing Highlights in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KatarzynaKruszynska.pdf PDF] |0:15 |---- |19:15 |Kris Rybicki |Update on Gaia19bld event |0:15 |---- |19:30 |Break | |0:15 |---- |19:45 |Zofia Kaczmarek |Lensing events with parallax in Gaia Alerts |0:15 |---- |20:00 |Marius Maskoliunas |Preliminary results for the microlensing event Gaia19dke [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MariusMaskoliunas.pdf PDF] |0:15 |---- |20:15 |Ashish Mahabal |ZTF, ML, and Variability |0:15 |---- |20:30 |Przemek Mroz |All-sky searches for gravitational microlensing events with data from the Zwicky Transient Facility |0:15 |---- |20:45 |Etienne Bachelet |The OMEGA Key Project : detection of cold planets and stellar remnants in the entire Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/EtienneBachelet.pdf PDF] |0:15 |---- | | | | |---- | | | | |---- |colspan="4"|<big>'''Thursday 21 January 2021'''</big> |---- |10:00 |Iair Arcavi |TDEs overview |0:15 |---- |10:15 |Nada Ihanec |Bowen Fluorescence Flares - new class of nuclear transients |0:05 |---- |10:20 |Szymon Kozlowski |Quasar Variability in Gaia: Simulation Perspective |0:15 |---- |10:35 |Morgan Fraser |Supernovae and Gaia |0:15 |---- |10:50 |Mateusz Bronikowski |Overluminous transients in Gaia Alerts using photometric redshift |0:05 |---- |10:55 |Benny Trakhtenbrot |Resolving the Mystery of Changing Look AGN with Responsive Follow-up Observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/BennyTrakhtenbrot.pdf PDF] |0:15 |---- |11:10 |Break | |0:30 |---- |11:40 |Tsvi Piran |TDEs in AGNs |0:15 |---- |11:55 |Nikolaos Mandarakas |Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NikosMandarakas.pdf PDF] |0:15 |---- |12:10 |Benito Marcote |Discovering radio transients from Gaia Alerts |0:15 |---- |12:25 |Dmitry Blinov |On the need of optical polarimetry follow up of flaring AGN in Gaia alerts |0:05 |---- |12:30 |Jaroslav Merc |Gaia18aen: First symbiotic star discovered by Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JaroslavMerc.pdf PDF] |0:15 |---- |12:45 |Michał Siwak |In search for new eruptive young stars among Gaia Alerts |0:15 |---- |13:00 |Artie Hatzes |The Alfred Jensch 2m Telescope and its Use for Targets of Opportunity |0:15 |---- |13:15 |Klaas Wiersema |A snapshot survey of polarised light in optical transients |0:15 |---- | | | | |---- |colspan="4"|<big>'''Friday 22 January 2021'''</big> |---- |15:05 |Gaspar Bakos |Monitoring the sky with HATPI |0:15 |---- |15:20 |Josep Manel Carrasco |Science alerts from the Joan Oró telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JosepManelCarrasco.pdf PDF] |0:05 |---- |15:25 |Marco Lam |First glimpse of the new LT/SPRAT automated pipeline with ASPIRED [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MarcoLam.pdf PDF] |0:05 |---- |15:30 |Stephen Brincat & Charles Galdies |Time-series photometry from Flarestar Observatory – Malta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/StephenBrincat.pdf PDF] |0:15 |---- |15:45 |Michel Dennefeld |Follow-up of some Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MichelDennefeld.pdf PDF] |0:15 |---- |16:00 |Break | |0:20 |---- |16:20 |Goran Damljanovic |Gaia Alerts and the Serbian-Bulgarian mini-network telescopes during 2020 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/GoranDamljanovic.pdf PDF] |0:15 |---- |16:35 |Justas Zdanavičius |Gaia alert observations and reductions in Lithuania |0:15 |---- |16:50 |Ruta Urbonaviciute |Search for variable stars in the northern sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RutaUrbonaviciute.pdf PDF] |0:05 |---- |16:55 |Algita Stankevičiūtė |Future of detecting Black Holes with ground-based telescopes |0:05 |---- |17:00 |Karsten Brogaard |Educational telescope at Mt. Kent |0:05 |---- |17:05 |Fraser Lewis |Linking Education and Research Using Robotic Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/FraserLewis.pdf PDF] |0:15 |---- |17:20 |Agnieszka Słowikowska |Orbital and physical parameters distributions of exoplanets in the light of Gaia DR2 catalogue |0:05 |---- | | Nariman Ismailov | Spectral and photometric observations of some transient Gaia alert objects in Shamakhy Observatory (not presented [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NarimanIsmailov.pdf PDF] | |---- |17:25 |Summary | |0:15 |---- | | | | |---- |17:40 |'''Social meeting on WonderMe''' | | |} d58be656048e42fd57e6341b2730d46d279a20d0 6 126 2609 652 2021-01-12T17:26:18Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda-draft.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2611 2609 2021-01-12T17:49:11Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda-draft.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2612 2611 2021-01-13T12:10:27Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda-draft.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 332 2615 2601 2021-01-13T16:08:56Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[Media:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. The workshop holds the honorary patronage of the [https://polsa.gov.pl/en/ Polish Space Agency (POLSA)]. [[File:logo_polsa_en.png]] 639a04ccaa829a4636fecaa8f2f15a008b152b87 2617 2615 2021-01-13T16:10:19Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[Media:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. The workshop holds the honorary patronage of the [https://polsa.gov.pl/en/ Polish Space Agency (POLSA)]. [[File:logo_polsa_en.png|right|100px|polsa]] 2abebfb8b685a99f4d34f4865e7928a871584419 2618 2617 2021-01-13T16:10:29Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[Media:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. The workshop holds the honorary patronage of the [https://polsa.gov.pl/en/ Polish Space Agency (POLSA)]. [[File:logo_polsa_en.png|right|300px|polsa]] b309c21185ba76f5eba4232fe2760f3cc03689c5 2624 2618 2021-01-13T18:26:23Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[File:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. The workshop holds the honorary patronage of the [https://polsa.gov.pl/en/ Polish Space Agency (POLSA)]. [[File:logo_polsa_en.png|right|300px|polsa]] 4e34f6262854fdf1c6783de2061d88d988c79b4b 2626 2624 2021-01-13T18:26:54Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[Media:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. The workshop holds the honorary patronage of the [https://polsa.gov.pl/en/ Polish Space Agency (POLSA)]. [[File:logo_polsa_en.png|right|300px|polsa]] b309c21185ba76f5eba4232fe2760f3cc03689c5 2627 2626 2021-01-13T18:27:36Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2020-small.png|right|450px|poster2020]] '''The eleventh OPTICON Gaia Science Alerts workshop will be held [[Workshop2020:logistics | online 18-22 January 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio, X-ray and high energy * new members of the telescope network * new photometric calibration server * organization of the follow-up * future of alerts and extension of Gaia ---- * [[workshop2020:rationale|Rationale]] * [[workshop2020:agenda|Agenda]] * [[workshop2020:registration|Registration]] * [[workshop2020:logistics|Logistical information]] * [[Media:Poster2020.pdf|Poster for download]] <!-- * [[workshop2020:poster|Workshop's poster for download]] --> ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Marius Maskoliunas (Vilnius) * Kasia Kruszynska (Warsaw) * Nada Ihanec (Warsaw) * Gerry Gilmore (Cambridge) The workshop is supported jointly by the EC H2020 OPTICON grant no 730890 and Lithuanian RC DAINA grant no S-LL-19-2. The workshop holds the honorary patronage of the [https://polsa.gov.pl/en/ Polish Space Agency (POLSA)]. ddcf056b07b636e8e1109e6f89cb043d93036cf5 6 340 2616 2021-01-13T16:09:35Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 339 2622 2600 2021-01-13T18:25:09Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2020-small.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2623 2622 2021-01-13T18:25:37Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2020-small.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 338 2625 2599 2021-01-13T18:26:40Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2020.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 341 2631 2021-01-17T06:37:44Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 342 2633 2021-01-17T06:38:37Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2644 2633 2021-01-18T14:30:15Z Nada.ihanec 43 Nada.ihanec uploaded a new version of [[File:Abstracts2020.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2645 2644 2021-01-18T14:31:57Z Nada.ihanec 43 Nada.ihanec uploaded a new version of [[File:Abstracts2020.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 334 2656 2655 2021-03-04T05:42:42Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Agenda == <big> [https://docs.google.com/spreadsheets/d/1P2E7XcbXQfLw-RbKk6NwDjbCqch64iqfrQHOgTOE_NU/edit?usp=sharing Workshop Agenda as Google Spreadsheet] </big> <big> [[Media:Abstracts2020.pdf|Abstracts book]] </big> Throughout all days of the Workshop, the informal discussions can be carried out using [https://www.wonder.me/ Wonder] tool and Slack. The links will be provided to the registered participants. <!--- === Time table and YouTube stream === ---- {| class="wikitable" |---- |day/start time |UT |New Zealand |Japan |India |'''Europe''' |UK |New York |Los Angeles |YouTube |---- |Monday 18.Jan |2pm |(+1d ) 2am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |5pm |(+1d) 6am |(+1d) 2am |10:30pm |'''6pm''' |5pm |12pm |9am |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |9am |10pm |6pm |2:30pm |'''10am''' |9am |4am |1am |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |2pm |(+1d)3am |11pm |7:30pm |'''3pm''' |2pm |9am |6am |https://youtu.be/K2HIIKAfut8 |---- |} ---- ---> === Video Recordings === ---- {| class="wikitable" |---- |day |YouTube link |---- |Monday 18.Jan |https://youtu.be/BpNbkseqUBI |---- |Tuesday 19.Jan |https://youtu.be/8GNIXyMLGyc |---- |Wednesday 20.Jan |https://youtu.be/d88hjDmHX04 |---- |Thursday 21.Jan |https://youtu.be/Wylsoi_nUOU |---- |Friday 22.Jan |https://youtu.be/K2HIIKAfut8 |---- |} ---- == Agenda and slides == ---- {| class="wikitable" | |''name'' |''title'' |''duration (with discussion)'' |---- |---- |colspan="4"|<big>'''Monday 18 January 2021'''</big> |---- |15:00 |Lukasz Wyrzykowski |Welcome and technical information |0:05 |---- |15:05 |Marek Moszyński |Welcome address from the President of the Polish Space Agency |0:05 |---- |15:10 |Timo Prusti |Gaia overview [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:30 |---- |15:40 |Simon Hodgkin |Gaia Science Alerts: Status of the system [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/SimonHodgkin.pdf PDF] |0:25 |---- |16:05 |Gerry Gilmore |Gaia, OPTICON, ORP and time-domain astronomy |0:25 |---- |16:30 |John Davies |TDA in the OPTICON Radionet PILOT |0:15 |---- |16:45 |Harro Verkouter |ORP - PILOT = TOM + EVN |0:15 |---- |17:00 |Break | |0:15 |---- |17:15 |Lukasz Wyrzykowski |Introduction to the Black Hole Target Observation Manager (BHTOM) |0:15 |---- |17:30 |Maja Jabłońska |Black Hole Target Observation Manager |0:15 |---- |17:45 |Paweł Zieliński |Uploading data to BHTOM [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski.pdf PDF] |0:15 |---- |18:00 |Przemysław Mikołajczyk |CCDPhot for automated photometric processing |0:15 |---- |18:15 |Mikołaj Kałuszyński |Webservices in scientific applications, CCDPHOTsvc |0:15 |---- |18:30 |Rachel Street |Software tools to enhance alert-based science [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RachelStreet.pdf PDF] |0:05 |---- | | | | |---- |colspan="4"|<big>'''Tuesday 19 January 2021'''</big> |---- |10:00 |Pawel Zielinski |Spectroscopic classification of Gaia microlensing event candidates [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-spec.pdf PDF] |0:15 |---- |10:15 |Gábor Marton |Classification of Gaia Alerts with machine learning algorithms |0:15 |---- |10:30 |Ilknur Gezer |Photometric classification of Gaia microlensing event candidates with machine learning methods |0:15 |---- |10:45 |Roberto Alexander Cerviño |Automatic classification of Gaia Photometric Alerts using spectra data through Machine Learning and Deep Learning. |0:15 |---- |11:00 |Nicholas Rattenbury |New Zealand Time Critical Astrophysics |0:15 |---- |11:15 |Takahiro Sumi |PRIME |0:15 |---- |11:30 |Maria Gabriela Navarro |VVV Microlensing events in the Galactic bulge |0:15 |---- |11:45 |Akihiko Fukui |Photometry of Gaia Microlensing Events from Tomo-e Gozen Survey |0:05 |---- |11:50 |Break | |0:25 |---- |12:15 |Eran Ofek |The Large Array Survey Telescope and time delay estimation |0:30 |---- |12:45 |Mariusz Gromadzki |OGLE-IV Transient Search |0:15 |---- |13:00 |Zuzanna Kostrzewa-Rutkowska |Electromagnetic counterparts of gravitational wave sources with Gaia |0:15 |---- |13:15 |Hasan H. Esenoglu |Spectroscopy and Photometry of Gaia20eld (Nova Cas 2020) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/HasanEsenoglu.pdf PDF] |0:15 |---- |13:30 |Krzysztof Kaminski |Science with RBT/PST2 and PST3 telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KrzysztofKaminski.pdf PDF] |0:15 |---- |13:45 |Zsofia Nagy |Dipper-like variability of the Gaia alerted young star V555 Ori |0:15 |---- | | | | |---- |18:00 |WonderMe platform |Hands-on in data uploading in BHTOM led by Pawel Zielinski [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/PawelZielinski-handson.pdf PDF] | |---- | | | | |---- |colspan="4"|<big>'''Wednesday 20 January 2021'''</big> |---- | | | | |---- |15:00 |Zoom |Hands-on in data uploading in BHTOM led by Pawel Zielinski (repeated) | |---- | | | | |---- |18:00 |Nami Mowlavi |Overview of variable objects processing within the Gaia consortium [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NamiMowlavi.pdf PDF] |0:25 |---- |18:25 |William Thuillot |Gaia follow-up of the uncatalogued Solar System Objects [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/WilliamThuillot.pdf PDF] |0:15 |---- |18:40 |Dirk Froebrich |Gaia Alert Follow up with the HOYS Citizen Science project |0:15 |---- |18:55 |Malhar Kendurkar |Data Analysis and Search for Astronomical Transients (AT's) [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MalharKendurkar.pdf PDF] |0:05 |---- |19:00 |Katarzyna Kruszyńska |Microlensing Highlights in Gaia Science Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/KatarzynaKruszynska.pdf PDF] |0:15 |---- |19:15 |Kris Rybicki |Update on Gaia19bld event |0:15 |---- |19:30 |Break | |0:15 |---- |19:45 |Zofia Kaczmarek |Lensing events with parallax in Gaia Alerts |0:15 |---- |20:00 |Marius Maskoliunas |Preliminary results for the microlensing event Gaia19dke [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MariusMaskoliunas.pdf PDF] |0:15 |---- |20:15 |Ashish Mahabal |ZTF, ML, and Variability |0:15 |---- |20:30 |Przemek Mroz |All-sky searches for gravitational microlensing events with data from the Zwicky Transient Facility |0:15 |---- |20:45 |Etienne Bachelet |The OMEGA Key Project : detection of cold planets and stellar remnants in the entire Milky Way [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/EtienneBachelet.pdf PDF] |0:15 |---- | | | | |---- | | | | |---- |colspan="4"|<big>'''Thursday 21 January 2021'''</big> |---- |10:00 |Iair Arcavi |TDEs overview |0:15 |---- |10:15 |Nada Ihanec |Bowen Fluorescence Flares - new class of nuclear transients |0:05 |---- |10:20 |Szymon Kozlowski |Quasar Variability in Gaia: Simulation Perspective |0:15 |---- |10:35 |Morgan Fraser |Supernovae and Gaia |0:15 |---- |10:50 |Mateusz Bronikowski |Overluminous transients in Gaia Alerts using photometric redshift |0:05 |---- |10:55 |Benny Trakhtenbrot |Resolving the Mystery of Changing Look AGN with Responsive Follow-up Observations [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/BennyTrakhtenbrot.pdf PDF] |0:15 |---- |11:10 |Break | |0:30 |---- |11:40 |Tsvi Piran |TDEs in AGNs |0:15 |---- |11:55 |Nikolaos Mandarakas |Search for AGN counterparts of unidentified Fermi-LAT sources with optical polarimetry. Demonstration of the technique [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NikosMandarakas.pdf PDF] |0:15 |---- |12:10 |Benito Marcote |Discovering radio transients from Gaia Alerts |0:15 |---- |12:25 |Dmitry Blinov |On the need of optical polarimetry follow up of flaring AGN in Gaia alerts |0:05 |---- |12:30 |Jaroslav Merc |Gaia18aen: First symbiotic star discovered by Gaia [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JaroslavMerc.pdf PDF] |0:15 |---- |12:45 |Michał Siwak |In search for new eruptive young stars among Gaia Alerts |0:15 |---- |13:00 |Artie Hatzes |The Alfred Jensch 2m Telescope and its Use for Targets of Opportunity |0:15 |---- |13:15 |Klaas Wiersema |A snapshot survey of polarised light in optical transients |0:15 |---- | | | | |---- |colspan="4"|<big>'''Friday 22 January 2021'''</big> |---- |15:05 |Gaspar Bakos |Monitoring the sky with HATPI |0:15 |---- |15:20 |Josep Manel Carrasco |Science alerts from the Joan Oró telescope [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/JosepManelCarrasco.pdf PDF] |0:05 |---- |15:25 |Marco Lam |First glimpse of the new LT/SPRAT automated pipeline with ASPIRED [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MarcoLam.pdf PDF] |0:05 |---- |15:30 |Stephen Brincat & Charles Galdies |Time-series photometry from Flarestar Observatory – Malta [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/StephenBrincat.pdf PDF] |0:15 |---- |15:45 |Michel Dennefeld |Follow-up of some Gaia Alerts [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/MichelDennefeld.pdf PDF] |0:15 |---- |16:00 |Break | |0:20 |---- |16:20 |Goran Damljanovic |Gaia Alerts and the Serbian-Bulgarian mini-network telescopes during 2020 [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/GoranDamljanovic.pdf PDF] |0:15 |---- |16:35 |Justas Zdanavičius |Gaia alert observations and reductions in Lithuania |0:15 |---- |16:50 |Ruta Urbonaviciute |Search for variable stars in the northern sky [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/RutaUrbonaviciute.pdf PDF] |0:05 |---- |16:55 |Algita Stankevičiūtė |Future of detecting Black Holes with ground-based telescopes |0:05 |---- |17:00 |Karsten Brogaard |Educational telescope at Mt. Kent |0:05 |---- |17:05 |Fraser Lewis |Linking Education and Research Using Robotic Telescopes [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/FraserLewis.pdf PDF] |0:15 |---- |17:20 |Agnieszka Słowikowska |Orbital and physical parameters distributions of exoplanets in the light of Gaia DR2 catalogue |0:05 |---- | | Nariman Ismailov | Spectral and photometric observations of some transient Gaia alert objects in Shamakhy Observatory (not presented [http://www.astrouw.edu.pl/~wyrzykow/GAIA/GSAW2020/NarimanIsmailov.pdf PDF] | |---- |17:25 |Summary | |0:15 |---- | | | | |---- |17:40 |'''Social meeting on WonderMe''' | | |} 420a1c12959abacc54dcba0b14ae434d517afd79 8 3 2657 2547 2021-07-14T10:23:07Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2021 **workshop2021:main|Main Workshop Page **workshop2021:rationale|Rationale **workshop2021:agenda|Program **workshop2021:registration|Participants and Registration **workshop2021:logistics|Logistics *workshop 2020 **workshop2020:main|Main Workshop Page **workshop2020:agenda|Archive of presentations *workshop 2019 **workshop2019:main|Main Workshop Page **workshop2019:agenda|Archive of presentations *workshop 2018 **workshop2018:main|Main Workshop Page **workshop2018:agenda|Archive of presentations *workshop 2017 **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 381ad952feeae668546231025781732b4e36d886 2658 2657 2021-07-14T10:23:30Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2021 **workshop2021:main|Main Workshop Page **workshop2021:rationale|Rationale **workshop2021:agenda|Program **workshop2021:registration|Participants and Registration **workshop2021:logistics|Logistics *workshop 2020 (archive) **workshop2020:main|Main Workshop Page **workshop2020:agenda|Archive of presentations *workshop 2019 (archive) **workshop2019:main|Main Workshop Page **workshop2019:agenda|Archive of presentations *workshop 2018 (archive) **workshop2018:main|Main Workshop Page **workshop2018:agenda|Archive of presentations *workshop 2017 (archive) **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 (archive) **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 (archive) **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 773335bb54ada2472ac66bcbe1968c75375cc050 0 343 2659 2021-07-14T10:27:59Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The First ORP Time-Domain meeting and 12th Gaia Science Alerts workshop will be held in Workshop2021:..." wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The First ORP Time-Domain meeting and 12th Gaia Science Alerts workshop will be held in [[Workshop2021:logistics | FORTH/Crete and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719 and Lithuanian RC DAINA grant no S-LL-19-2. 677f6d00af3de7abd2637c49cd2940bba09b9d33 2665 2659 2021-07-14T17:39:12Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The First ORP Time-Domain meeting and 12th Gaia Science Alerts workshop will be held in [[Workshop2021:logistics | FORTH/Crete and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 6596f99d7c89aae4931d9a48587e18b7228f2923 2672 2665 2021-07-20T12:03:45Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The First ORP Time-Domain meeting and 12th Gaia Science Alerts workshop will be held at the premisses of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 46b638f4894fef039a177cfe4d2402a6a4f90c13 2678 2672 2021-09-02T12:30:33Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[Media:Poster2021-small.png|right|450px|poster2021]] '''The First ORP Time-Domain meeting and 12th Gaia Science Alerts workshop will be held at the premisses of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 12aebec9e7ce88d237235034e750ceada8ea124d 2679 2678 2021-09-02T12:30:59Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The First ORP Time-Domain meeting and 12th Gaia Science Alerts workshop will be held at the premisses of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 46b638f4894fef039a177cfe4d2402a6a4f90c13 2681 2679 2021-09-03T12:42:49Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 9a587d81494e83b6db09d2c378f21d78e5424abb 2683 2681 2021-09-07T08:40:00Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[File:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 033dfcdb7b5b99b8c7599611cb9916211ae4abc8 2685 2683 2021-09-07T08:40:23Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|450px|poster2021]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 9a587d81494e83b6db09d2c378f21d78e5424abb 0 1 2660 2563 2021-07-14T10:28:58Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2021:main|12th Gaia Science Alerts Workshop 2021, FORTH/Crete, 8-12 November 2021]]</Big>''' </center> ---- <center> [[Workshop2020:main|11th Gaia Science Alerts Workshop 2020, on-line - archive of presentations]] [[Workshop2019:main|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:main|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:main|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 77fab49a06f943a34b0dc374073da6fa7ec97116 0 344 2661 2021-07-14T10:52:46Z Gsawgwikiadmin 1 Created page with "<big>'''[LINK Registration is now OPEN]'''</big> ''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please..." wikitext text/x-wiki <big>'''[LINK Registration is now OPEN]'''</big> ''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.'' ''Please note that due to uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line.'' 15463fd9cf933320e9db7aa478ac183d50db0748 2662 2661 2021-07-14T10:53:11Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[LINK Registration is now OPEN]'''</big> '''''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''''' ''Please note that due to uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line.'' d068a574eeb98b4fe3a4ed195e54f6b995686e25 2663 2662 2021-07-14T10:53:29Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[LINK Registration is now OPEN]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' Please note that due to uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. d87b8b5ada59cdeaa76536c27e503a1a537ba84d 2664 2663 2021-07-14T14:37:37Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is now OPEN]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' Please note that due to uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. a553e908793750635758f80d09d7ce7c46aa6fd5 2676 2664 2021-07-29T05:55:00Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' Please note that due to uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. 044deb63087f29c4364f19dd837b07538427251b 2687 2676 2021-09-08T07:50:40Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' 53c6d8a6a21a88c8eb7c68022d837dd3d59552aa 2705 2687 2021-10-20T10:38:47Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University, Poland 0cf2c9a26e58564a887962447812097c273d88b8 0 345 2666 2021-07-14T17:41:28Z Gsawgwikiadmin 1 Created page with "''In order to facilitate online attendance for participants from a range of time zones, we plan the in-person meeting to be held at varying half-days over the scheduled 5 days.''" wikitext text/x-wiki ''In order to facilitate online attendance for participants from a range of time zones, we plan the in-person meeting to be held at varying half-days over the scheduled 5 days.'' c959089bd29b1dbb4c162924c4c08f7ca788e19e 2667 2666 2021-07-14T17:42:23Z Gsawgwikiadmin 1 wikitext text/x-wiki The agenda of the workshop will be composed based on the talks suggested by the registrants. ''In order to facilitate online attendance for participants from a range of time zones, we plan the in-person meeting to be held at varying half-days over the scheduled 5 days.'' 84726f6cbf1df4d45f36803b7d498f3025835c33 2669 2667 2021-07-14T17:44:08Z Gsawgwikiadmin 1 wikitext text/x-wiki The agenda of the workshop will be composed based on the talks suggested by the registrants. We anticipate to start on Monday 8th Nov with the lunch and finish on Friday with the lunch. ''In order to facilitate online attendance for participants from a range of time zones, we plan the in-person meeting to be held at varying half-days over the scheduled 5 days.'' bd8e13a2d700163891bd9f07b7f76bdfa4ad4ddc 2670 2669 2021-07-14T17:44:17Z Gsawgwikiadmin 1 wikitext text/x-wiki The agenda of the workshop will be composed based on the talks suggested by the registrants. We anticipate to start on Monday 8th Nov with the lunch and finish on Friday 12th Nov with the lunch. ''In order to facilitate online attendance for participants from a range of time zones, we plan the in-person meeting to be held at varying half-days over the scheduled 5 days.'' 6ccc8294e39b1931e15d2fe208ab41fa21359587 0 346 2668 2021-07-14T17:43:20Z Gsawgwikiadmin 1 Created page with "The workshop will be held at the [https://www.forth.gr/ FORTH institute], Crete." wikitext text/x-wiki The workshop will be held at the [https://www.forth.gr/ FORTH institute], Crete. e45d2f26936c15147a926a2a53fe0cbf82b3f48f 2671 2668 2021-07-14T17:45:01Z Gsawgwikiadmin 1 wikitext text/x-wiki The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. 1760fad66b3eb418354f76fa00f885604a4f2fd3 2688 2671 2021-10-08T10:36:29Z Kruszynska.katarzyna.oauw 47 wikitext text/x-wiki = Workshop Venue = The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] = Accomodation = List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] 0f0d04bf178f85c17ebd20872070a55bb019aa19 2689 2688 2021-10-08T10:40:21Z Kruszynska.katarzyna.oauw 47 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] e87c48ed8c813a010d274161fc6d3b6c6c9c8ec5 2690 2689 2021-10-08T10:43:00Z Kruszynska.katarzyna.oauw 47 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] 538120c7f039d4929a382dc81d54c489c4633a70 2691 2690 2021-10-08T10:50:30Z Kruszynska.katarzyna.oauw 47 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € 26334f78be172f54a159811e65f3d0c284509f07 2692 2691 2021-10-08T10:51:20Z Kruszynska.katarzyna.oauw 47 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € 1258d3d9428fde31c824a66bfd1fc21d0dfdb0e2 2693 2692 2021-10-08T10:54:10Z Kruszynska.katarzyna.oauw 47 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) 7b5b28e688b31bae03481b14731563d4e9ba52cd 2694 2693 2021-10-08T11:11:58Z Kruszynska.katarzyna.oauw 47 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € 967585753841fcc39ad1547ebe3dd6bc4a6bb4e7 2695 2694 2021-10-08T11:15:46Z Kruszynska.katarzyna.oauw 47 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 350fe8d699ebfd94696899552fd242599a609e7b 2696 2695 2021-10-18T12:07:38Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We suggest to all people attending in-person to select the same hotel, for easier commuting and meeting: * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 5b67a2312c21f792c7cb93ef739857bff1f51dd1 2697 2696 2021-10-18T12:08:02Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We suggest to all people attending in-person to select the same hotel, for easier commuting and meeting: * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) '''75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 fax: +30 2810 211211 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € ''' ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 96a878a91aef92294a6cc2148991313877a8bb72 2698 2697 2021-10-18T12:08:37Z Gsawgwikiadmin 1 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We suggest to all people attending in-person to select the same hotel, for easier commuting and meeting: * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) '''75, Dimokratias Street, 71306 Heraklion''' '''tel.: +30 2810 238812''' '''URL: www.galaxy-hotel.com/en/''' '''e-mail: galaxy@economouhotels.com''' '''Single room: from 60.00 €''' '''Double room: 85.00 €''' ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 0ddd7ed4800e1d02b5e7e1ef6d02d8e349910202 2699 2698 2021-10-18T12:08:48Z Gsawgwikiadmin 1 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We suggest to all people attending in-person to select the same hotel, for easier commuting and meeting: * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) '''75, Dimokratias Street, 71306 Heraklion''' '''tel.: +30 2810 238812''' '''URL: www.galaxy-hotel.com/en/''' '''e-mail: galaxy@economouhotels.com''' '''Single room: from 60.00 €''' '''Double room: 85.00 €''' ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 6d28335230be95452130494b4a0d7ba8012fc7c9 2700 2699 2021-10-18T12:09:03Z Gsawgwikiadmin 1 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We suggest to all people attending in-person to select the same hotel, for easier commuting and meeting: * <big>'''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****)</big> '''75, Dimokratias Street, 71306 Heraklion''' '''tel.: +30 2810 238812''' '''URL: www.galaxy-hotel.com/en/''' '''e-mail: galaxy@economouhotels.com''' '''Single room: from 60.00 €''' '''Double room: 85.00 €''' ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 18c63624fd3bc3c42d1b8bca5016a1d9f40b52d9 2701 2700 2021-10-19T10:54:15Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 88b97903091e4d02cda13be545b162973da8b930 2702 2701 2021-10-19T10:54:23Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 fax: +30 2810 226265 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 6faefe1664ce7fde3fbb12be89fb2ca9d5306d8a 2703 2702 2021-10-20T10:33:15Z Gsawgwikiadmin 1 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * '''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****) 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 0f139152fdbb46ad93155c6a7b3e212d12c9ad5b 2704 2703 2021-10-20T10:33:34Z Gsawgwikiadmin 1 /* Accomodation */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * <big>'''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****)</big> 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € e20cf1f755190522c9c4dc7023041ede7083c242 0 347 2673 2021-07-20T12:07:02Z Gsawgwikiadmin 1 Created page with "=== Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and phot..." wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometric data, and Gaia Photometric Science Alerts continues as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Gaia Alerts Science === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 12th in the series, will be an opportunity to learn about the current state (and future plans for) Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia Alerts, and we will explore the scientific potential of the programme. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner followup observations of transient alerts reported by other (non-GAIA) facilities. === Multimessenger time-domain
 === In particular, we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increase the scientific output of surveys and follow-up observations in the multi-messenger era. ef09512583cd9a66d6b44bc2b3fa42e888b9d174 2674 2673 2021-07-21T06:27:52Z Gsawgwikiadmin 1 wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometric data, and Gaia Photometric Science Alerts continues as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Gaia Alerts Science === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 12th in the series, will be an opportunity to learn about the current state (and future plans for) Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia Alerts, and we will explore the scientific potential of the programme. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities. === Multimessenger time-domain
 === In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. === Meeting in the Covid era === The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be - at least for some participants - an in-person meeting. We have all learned the benefits of on-line meetings for global participation so will schedule sessions during the week at times suitable for the widest possible participation on-line. You are asked in the Registration to state your preference for in-person - if we are able to host that - or on-line participation. We shall certainly host on-line participation. Given the ever-changing Covid, travel restriction and post-travel quarantine requirements, we will make a final decision on in-person participation in early-mid October. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place. 80af636d1945139ba5baf4d93daecc403c161813 2675 2674 2021-07-21T06:28:14Z Gsawgwikiadmin 1 wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. DPAC have just released EDR3 with unprecedented astrometric and photometric data, and Gaia Photometric Science Alerts continues as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Gaia Alerts Science === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 12th in the series, will be an opportunity to learn about the current state (and future plans for) Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia Alerts, and we will explore the scientific potential of the programme. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities. === Multimessenger time-domain
 === In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. === Meeting in the Covid era === The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be - at least for some participants - an in-person meeting. We have all learned the benefits of on-line meetings for global participation so will schedule sessions during the week at times suitable for the widest possible participation on-line. You are asked in the Registration to state your preference for in-person - if we are able to host that - or on-line participation. We shall certainly host on-line participation. Given the ever-changing Covid, travel restriction and post-travel quarantine requirements, we will make a final decision on in-person participation in early-mid October. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place. 915378827e78cae694beb8fc5a37312ec384d6be 6 348 2677 2021-09-02T12:30:07Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2682 2677 2021-09-07T08:39:36Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2021-small.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2686 2682 2021-09-07T08:42:21Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2021-small.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 349 2680 2021-09-02T12:31:14Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2684 2680 2021-09-07T08:40:12Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2021.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 344 2706 2705 2021-10-20T10:39:09Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University, Poland 6f53fcf19c53917846d4c47c180c638260e5cceb 2707 2706 2021-10-20T10:40:32Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # Siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University, Poland 88b33cf744f48b399aa5e8bdc3d8b09922995b9a 2708 2707 2021-10-21T11:01:14Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # Siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University, Poland a13761404b0f8b424140d33414f4d416fbdb6267 2709 2708 2021-10-21T16:01:24Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 638bcac0ec188f3f6a1f9105ca8832fab1a5d489 2710 2709 2021-10-22T10:36:18Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 61e324b9b74c85569dfc7e4ab57efe8d8fadfb27 2711 2710 2021-10-25T05:43:17Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Simon Hodgkin, Institute of Astronomy, Cambridge University # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 1cc296a2fe3ae0e096019ff908c8f2a53e03da59 2713 2711 2021-10-25T15:12:49Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Josep Manel Carrasco, Institut de Ciències del Cosmos - Universitat de Barcelona # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Bob Eldering, Joint Institute for VLBI ERIC # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Simon Hodgkin, Institute of Astronomy, Cambridge University # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University a93056e6ebf9554ca3a841afae85ad12e1b0698d 2714 2713 2021-10-28T05:26:24Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Karolina Bąkowska, N. Copernicus University # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Josep Manel Carrasco, Institut de Ciències del Cosmos - Universitat de Barcelona # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Bob Eldering, Joint Institute for VLBI ERIC # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Simon Hodgkin, Institute of Astronomy, Cambridge University # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 807c3a8c51fcf57ef7faa9f1b037a6530067d4dc 2720 2714 2021-10-30T20:28:58Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Karolina Bąkowska, N. Copernicus University # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Josep Manel Carrasco, Institut de Ciències del Cosmos - Universitat de Barcelona # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Bob Eldering, Joint Institute for VLBI ERIC # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Simon Hodgkin, Institute of Astronomy, Cambridge University # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # Siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 00565f79dd3e4b5453d3201c207d6e72f2951c83 2721 2720 2021-11-02T10:05:40Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Karolina Bąkowska, N. Copernicus University # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Josep Manel Carrasco, Institut de Ciències del Cosmos - Universitat de Barcelona # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Michel Dennefeld, IAP/Paris and Sorbonne University # Bob Eldering, Joint Institute for VLBI ERIC # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Simon Hodgkin, Institute of Astronomy, Cambridge University # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, ilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 52d156429f48beac5406b7d823841c26ba9eec5a 0 345 2712 2670 2021-10-25T15:04:36Z Gsawgwikiadmin 1 wikitext text/x-wiki The agenda of the workshop will be composed based on the talks suggested by the registrants. We anticipate to start on Monday 8th Nov with the lunch and finish on Friday 12th Nov with the lunch. ''In order to facilitate online attendance for participants from a range of time zones, we plan the in-person meeting to be held at varying half-days over the scheduled 5 days.'' Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Wed or Thu. c216959e59e5d5323c48f7ec28565b8ab3cc35ba 2715 2712 2021-10-29T14:22:37Z Gsawgwikiadmin 1 wikitext text/x-wiki [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[Media:draft-agenda.pdf]] Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Wed or Thu. 9414517528ee7cd731a843f7ea82e24098298595 2717 2715 2021-10-29T14:23:14Z Gsawgwikiadmin 1 wikitext text/x-wiki [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[Media:draft-agenda.pdf Draft agenda in PDF]] Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Wed or Thu. 072be8211df2442b186781df858137b11d079c97 2718 2717 2021-10-29T14:23:25Z Gsawgwikiadmin 1 wikitext text/x-wiki [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[Media:draft-agenda.pdf| Draft agenda in PDF]] Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Wed. 48b29a427bfb7557e6eeb5c8011a9c9fd177d29f 2719 2718 2021-10-29T14:26:25Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[Media:draft-agenda.pdf| Draft agenda in PDF]] Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Wed. 6b8a111f5320053b44d0d3dd3929c5888f25c9ce 2723 2719 2021-11-03T06:38:22Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[Media:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 14:00] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 14:00] 6ce8a1eece56855650d283fcb0667027a990c8d3 2725 2723 2021-11-03T06:39:44Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[File:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 14:00] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 14:00] 48613d7818cffe72fbf24e10378ed19c571e41d6 2727 2725 2021-11-03T06:40:16Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- [https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] [[Media:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 14:00] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 14:00] 6ce8a1eece56855650d283fcb0667027a990c8d3 2728 2727 2021-11-03T06:40:35Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] </big> [[Media:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 14:00] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 14:00] 4017a5de012c9d90988333e4fb09d5463cc410e2 2729 2728 2021-11-03T06:40:53Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] </big> [[Media:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 14:00 CET] bed96dd349259e38b275311970f8e6e1b21ac2ed 2730 2729 2021-11-03T22:16:28Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] </big> [[Media:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 3b18ab90ca855107c03d80b231998385572d2c8f 2731 2730 2021-11-05T06:54:15Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] </big> [[File:draft-agenda.pdf| Draft agenda in PDF]] [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 4c8359b6396f2d67eed81739274a8a7e85da8676 2733 2731 2021-11-05T06:55:13Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Draft agenda on Google Spreadsheets] </big> [[Media:draft-agenda.pdf| Draft agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] f52421a397cb0ae1b176cf7cdecf5d90dc6b72b0 2734 2733 2021-11-05T06:55:35Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </big> [[Media:draft-agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 40a2c83e9e756613821fd6643a11abca1292711e 2735 2734 2021-11-05T06:55:52Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[Media:draft-agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 9f736827d87be0a91b2d8ca91409d75015cad710 2736 2735 2021-11-05T10:13:53Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 510622a0596700e053d2f8c7f60271c0810c0d76 2738 2736 2021-11-05T10:14:18Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[Media:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 4549f9695bd0b7d2f0cfc9c3d72b09b5a8392fb8 2739 2738 2021-11-07T20:05:24Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/2_bQ8y29_LQ YouTube Monday 8 Nov 2021 14:00 CET] [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 510622a0596700e053d2f8c7f60271c0810c0d76 2743 2739 2021-11-08T09:18:04Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 CET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 20ba6a3b0a3c34253bb5764a0d3c1b0c097638cf 2744 2743 2021-11-08T12:12:02Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 CET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 CET] 261b33053c4bb3d512c0d62c6ecd25148bd3a9d2 2748 2744 2021-11-09T08:38:17Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 EET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 EET] [https://youtu.be/0GVdi47pk1M YouTube Tuesday 9 Nov 2021 17:00 EET) for Bryan Holler talk [http://astrouw.edu.pl/~wyrzykow/SEM/sem211109.html Abstract] 9ceeadf8cc3c3b0e74566a43996ec1ab4089d820 2749 2748 2021-11-09T08:38:27Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 EET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 EET] [https://youtu.be/0GVdi47pk1M YouTube Tuesday 9 Nov 2021 17:00 EET] for Bryan Holler talk [http://astrouw.edu.pl/~wyrzykow/SEM/sem211109.html Abstract] eb198641397feb2985747337feab0c2ae762e7d5 2750 2749 2021-11-09T13:31:44Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 EET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 EET] [https://youtu.be/0GVdi47pk1M YouTube Tuesday 9 Nov 2021 17:00 EET] for Bryan Holler talk [http://astrouw.edu.pl/~wyrzykow/SEM/sem211109.html Abstract] [https://youtu.be/MVsZgfmA6tk YouTube Wednesday 10 Nov 2021 15:00 EET] 47dd897f42fc4468f2bd44bc0daf4dac3598c9d9 2751 2750 2021-11-09T13:31:56Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 EET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 EET] [https://youtu.be/0GVdi47pk1M YouTube Tuesday 9 Nov 2021 17:00 EET] for Bryan Holler talk [http://astrouw.edu.pl/~wyrzykow/SEM/sem211109.html Abstract] [https://youtu.be/MVsZgfmA6tk YouTube Wednesday 10 Nov 2021 15:00 EET] 1c076f1770a7a82ce66d0f6b0797395436e903e6 6 350 2716 2021-10-29T14:22:57Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2726 2716 2021-11-03T06:40:04Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Draft-agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2732 2726 2021-11-05T06:54:34Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Draft-agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 346 2722 2704 2021-11-02T12:46:45Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. '''The meeting room is "Orfanoudakis" Seminar Room.''' Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * <big>'''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****)</big> 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 337b322420679c6157402ccf2d0473bd18ebd600 2724 2722 2021-11-03T06:38:42Z Gsawgwikiadmin 1 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. '''The meeting room is "Orfanoudakis" Seminar Room.''' Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == Workshop Dinner == Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Thursday. == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * <big>'''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****)</big> 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 0c71fc2b29c389a1e9dbc720e3f708100c1ed17f 2745 2724 2021-11-08T14:19:31Z Kruszynska.katarzyna.oauw 47 wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. '''The meeting room is "Orfanoudakis" Seminar Room.''' Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == Workshop Dinner == Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Thursday. == Extracurricular activities == * Museums Heraklion Archaeological Museum [https://heraklionmuseum.gr/?page_id=1406&lang=en] Historical Museum of Crete [https://www.historical-museum.gr/eng/] Palace of Knossos [https://www.heraklion.gr/en/ourplace/knossos/knossos.html] * Recommended Restaurants There are many excellent options for dining in Heraklion. Here are some suggestions of favorites in the city center from the local comity. 1. Kouzineri (high quality steak house) [https://kouzeineri.com/en/] [https://www.tripadvisor.com/Restaurant_Review-g189417-d2223553-Reviews-Kouzeineri-Heraklion_Crete.html] 2. Plani (small traditional Greek/Cretan cuisine) [https://www.tripadvisor.com/Restaurant_Review-g189417-d5982408-Reviews-Plani-Heraklion_Crete.html] 3. Peskesi (more elaborate Cretan cuisine) [https://www.tripadvisor.com/Restaurant_Review-g189417-d6513925-Reviews-Peskesi-Heraklion_Crete.html] 4. Kukuvagia (many Cretan selections - tapas style dishes) [https://koukouvagiaher.gr/?lang=en] [https://www.tripadvisor.com/Restaurant_Review-g189417-d6898812-Reviews-Koukouvagia_Heraklion-Heraklion_Crete.html] 5. Tempelis (simple unassuming cuisine - tapas style dishes) [https://www.tripadvisor.com/Restaurant_Review-g189417-d4594173-Reviews-Kafeneio_O_Tempelis-Heraklion_Crete.html] 6. Athali (Cretan cuisine focused mostly on meat) [htps://www.tripadvisor.com/Restaurant_Review-g189417-d13004429-Reviews-Athali-Heraklion_Crete.html] 7. Ippokampos (excellent seafood selection) [https://www.tripadvisor.com/Restaurant_Review-g189417-d1098956-Reviews-Ippokampos-Heraklion_Crete.html] 8. Paralia (excellent seafood selection) [https://www.tripadvisor.com/Restaurant_Review-g189417-d2154040-Reviews-Paralia_Seaside_Restaurant-Heraklion_Crete.html] 9. Prasin Aloga (great quality - reasonable prices) [https://www.tripadvisor.com/ShowUserReviews-g189417-d837447-r360435773-Prassin_Aloga-Heraklion_Crete.html] 10. Mare Coffee bar & food (breakfast, lunch, coffee and drinks) [https://www.tripadvisor.com/Restaurant_Review-g189417-d3530337-Reviews-Mare_coffee_bar_food-Heraklion_Crete.html] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * <big>'''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****)</big> 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € b94cfedd356551bf201ee1affae2814f41a7d02d 2746 2745 2021-11-08T14:20:16Z Kruszynska.katarzyna.oauw 47 /* Extracurricular activities */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. '''The meeting room is "Orfanoudakis" Seminar Room.''' Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == Workshop Dinner == Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Thursday. == Extracurricular activities == * '''Museums''' Heraklion Archaeological Museum [https://heraklionmuseum.gr/?page_id=1406&lang=en] Historical Museum of Crete [https://www.historical-museum.gr/eng/] Palace of Knossos [https://www.heraklion.gr/en/ourplace/knossos/knossos.html] * '''Recommended Restaurants''' There are many excellent options for dining in Heraklion. Here are some suggestions of favorites in the city center from the local comity. 1. Kouzineri (high quality steak house) [https://kouzeineri.com/en/] [https://www.tripadvisor.com/Restaurant_Review-g189417-d2223553-Reviews-Kouzeineri-Heraklion_Crete.html] 2. Plani (small traditional Greek/Cretan cuisine) [https://www.tripadvisor.com/Restaurant_Review-g189417-d5982408-Reviews-Plani-Heraklion_Crete.html] 3. Peskesi (more elaborate Cretan cuisine) [https://www.tripadvisor.com/Restaurant_Review-g189417-d6513925-Reviews-Peskesi-Heraklion_Crete.html] 4. Kukuvagia (many Cretan selections - tapas style dishes) [https://koukouvagiaher.gr/?lang=en] [https://www.tripadvisor.com/Restaurant_Review-g189417-d6898812-Reviews-Koukouvagia_Heraklion-Heraklion_Crete.html] 5. Tempelis (simple unassuming cuisine - tapas style dishes) [https://www.tripadvisor.com/Restaurant_Review-g189417-d4594173-Reviews-Kafeneio_O_Tempelis-Heraklion_Crete.html] 6. Athali (Cretan cuisine focused mostly on meat) [htps://www.tripadvisor.com/Restaurant_Review-g189417-d13004429-Reviews-Athali-Heraklion_Crete.html] 7. Ippokampos (excellent seafood selection) [https://www.tripadvisor.com/Restaurant_Review-g189417-d1098956-Reviews-Ippokampos-Heraklion_Crete.html] 8. Paralia (excellent seafood selection) [https://www.tripadvisor.com/Restaurant_Review-g189417-d2154040-Reviews-Paralia_Seaside_Restaurant-Heraklion_Crete.html] 9. Prasin Aloga (great quality - reasonable prices) [https://www.tripadvisor.com/ShowUserReviews-g189417-d837447-r360435773-Prassin_Aloga-Heraklion_Crete.html] 10. Mare Coffee bar & food (breakfast, lunch, coffee and drinks) [https://www.tripadvisor.com/Restaurant_Review-g189417-d3530337-Reviews-Mare_coffee_bar_food-Heraklion_Crete.html] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * <big>'''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****)</big> 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 62b5beeb207518987499204b0db8adfa89e2b123 2747 2746 2021-11-08T14:20:41Z Kruszynska.katarzyna.oauw 47 /* Extracurricular activities */ wikitext text/x-wiki == Workshop Venue == The workshop will be held in the [https://www.ia.forth.gr/ FORTH Institute of Astrophysics], Crete. '''The meeting room is "Orfanoudakis" Seminar Room.''' Directions on Google Maps: [https://www.google.com/maps/d/u/0/viewer?ll=35.321918901692435%2C25.119035185199724&z=14&mid=1I4hLSoLB1M1_PADRQKsDoZAUo7uDF8aZ link] == Workshop Dinner == Workshop Dinner in Parastiescrete [https://parastiescrete.gr/] on Thursday. == Extracurricular activities == * '''Museums''' Heraklion Archaeological Museum [https://heraklionmuseum.gr/?page_id=1406&lang=en] Historical Museum of Crete [https://www.historical-museum.gr/eng/] Palace of Knossos [https://www.heraklion.gr/en/ourplace/knossos/knossos.html] * '''Recommended Restaurants''' There are many excellent options for dining in Heraklion. Here are some suggestions of favorites in the city center from the local comity. 1. Kouzineri (high quality steak house) [https://kouzeineri.com/en/] [https://www.tripadvisor.com/Restaurant_Review-g189417-d2223553-Reviews-Kouzeineri-Heraklion_Crete.html] 2. Plani (small traditional Greek/Cretan cuisine) [https://www.tripadvisor.com/Restaurant_Review-g189417-d5982408-Reviews-Plani-Heraklion_Crete.html] 3. Peskesi (more elaborate Cretan cuisine) [https://www.tripadvisor.com/Restaurant_Review-g189417-d6513925-Reviews-Peskesi-Heraklion_Crete.html] 4. Kukuvagia (many Cretan selections - tapas style dishes) [https://koukouvagiaher.gr/?lang=en] [https://www.tripadvisor.com/Restaurant_Review-g189417-d6898812-Reviews-Koukouvagia_Heraklion-Heraklion_Crete.html] 5. Tempelis (simple unassuming cuisine - tapas style dishes) [https://www.tripadvisor.com/Restaurant_Review-g189417-d4594173-Reviews-Kafeneio_O_Tempelis-Heraklion_Crete.html] 6. Athali (Cretan cuisine focused mostly on meat) [https://www.tripadvisor.com/Restaurant_Review-g189417-d13004429-Reviews-Athali-Heraklion_Crete.html] 7. Ippokampos (excellent seafood selection) [https://www.tripadvisor.com/Restaurant_Review-g189417-d1098956-Reviews-Ippokampos-Heraklion_Crete.html] 8. Paralia (excellent seafood selection) [https://www.tripadvisor.com/Restaurant_Review-g189417-d2154040-Reviews-Paralia_Seaside_Restaurant-Heraklion_Crete.html] 9. Prasin Aloga (great quality - reasonable prices) [https://www.tripadvisor.com/ShowUserReviews-g189417-d837447-r360435773-Prassin_Aloga-Heraklion_Crete.html] 10. Mare Coffee bar & food (breakfast, lunch, coffee and drinks) [https://www.tripadvisor.com/Restaurant_Review-g189417-d3530337-Reviews-Mare_coffee_bar_food-Heraklion_Crete.html] == By Air == The closest airports that we recommend: * ''' [https://www.airport-heraklion.com/ Heraklion (HER)] ''': the closest to FORTH Institute == Accomodation == We recommend all attendees to use the same hotel to facilitate commuting and informal meetings: * <big>'''[https://www.theatlantishotel.gr Aquila ATLANTIS Hotel]''' 5 Star(*****)</big> 2 Igias Street, 71202 Heraklion tel.: +30 2810 229103 URL: www.theatlantishotel.gr e-mail: reserv@theatlantishotel.gr Single room: from 64.00 € Double room: 85.00 € (in land view), 93.00 € (sea view) ---- List of other available hotels: [https://www.physics.uoc.gr/content/hotels Link] * '''[https://www.galaxy-hotel.com/en/ GALAXY Hotel]''' 5 Star(*****) 75, Dimokratias Street, 71306 Heraklion tel.: +30 2810 238812 URL: www.galaxy-hotel.com/en/ e-mail: galaxy@economouhotels.com Single room: from 60.00 € Double room: 85.00 € * '''[https://www.gdmmegaron.gr GMD MEGARON Hotel]''' 5 Star(*****) 9 D. Beaufort, 71202 Heraklion tel.: +30 2810 305300 URL: www.gdmmegaron.gr e-mail: megaron@gdmmegaron.gr Single room: from 65.00 € (city view), from 95.00 € (sea view) Double room: from 75.00 € (city view), from 105.00 € (sea view) * '''[https://capsishotels.gr/astoria/en/home-astoria-2/ CAPSIS ASTORIA Hotel]''' 4 Star(****) 11 Eleftherias Square, 71202 Heraklion tel.: +30 2810 343080-2 fax: +30 2810 229078 URL: capsishotels.gr/astoria/en/home-astoria-2/ e-mail: info@astoriacapsis.gr Single room: from 62.00 € Double room: 66.00 € * '''[https://www.lato.gr/ Lato Boutique Hotel]''' 4 Star(****) 15 Epimenidou Street, 71202 Heraklion tel.: +30 2810 228103, 334955 fax: +30 2810 240350 URL: www.lato.gr e-mail: info@lato.gr Single room: from 50.00 € (city view), from 60.00 € (sea view) Double room: from 55.00 € (city view), from 60.00 € (sea view) * '''[https://www.olivegreenhotel.com OLIVE GREEN Hotel]''' 4 Star(****) Meramvelou & Idomeneos Street, 71202 Heraklion tel.: +30 2810 302900 URL: www.olivegreenhotel.com e-mail: reservations@olivegreenhotel.com Single room: 55.00 €, 65.00 € (park view) Double room: 60.00 €, 65.00 € (park view) * '''[http://ibis-styles-heraklion-central.hotelscrete.net/en/ IBIS Styles Hotel]''' 4 Star(****) 26 Koroneou Street, 71202 Heraklion tel.: +30 2810 282020 URL: ibis-styles-heraklion-central.hotelscrete.net/en/ e-mail: HA9P7-RE@accor.gr Single room: from 57.00 € (city view), from 80.00 € (sea view) Double room: from 67.00 € (city view), from 90.00 € (sea view) * '''[https://www.atrion.gr/en ATRION Hotel]''' 4 Star(****) 9 Chronaki Street, 71202 Heraklion tel.: +30 2810 246000 fax: +30 2810 223292 URL: www.atrion.gr e-mail: info@atrion.gr Single room: 55.00 € Double room: 77.00 € * '''[https://www.hotelolympic.com/ Hotel OLYMPIC]''' 3 Star(***) Kornarou Square, 71201 Heraklion tel.: +30 2810 288861 fax: +30 2810 222512 URL: www.hotelolympic.com e-mail: info@hotelolympic.com Single room: 46.00 € Double room: 60.00 € * '''[https://www.kastro-hotel.gr/ KASTRO Hotel]''' 3 Star(***) 17 Theotokopoulou Street, 71202 Heraklion tel.: +30 2810 285020 fax: +30 2810 223622 URL: www.kastro-hotel.gr e-mail: info@kastro-hotel.gr Single room: 45.00 € Double room: 55.00 € * '''[https://www.elgrecohotel.gr/en/ EL GRECO Hotel]''' 2 Star(**) 4 1821th Street, 71202 Heraklion tel.: +30 2810 281071-5 fax: +30 2810 281072 URL: www.elgrecohotel.gr email: elgrecohotel@her.forthnet.gr Single room: 35.00 € Double room: 45.00 € 0b2413bb4adcd93aaa465a5e9be559f9ee56fae4 6 325 2737 2493 2021-11-05T10:14:07Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2740 2737 2021-11-07T20:05:56Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2741 2740 2021-11-07T20:35:49Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2742 2741 2021-11-08T09:17:43Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2752 2742 2021-11-09T15:28:08Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 343 2753 2685 2021-11-10T15:53:46Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|350px|poster2021]] [[File:GroupPhoto1.jpg|right|400px|groupphoto1]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 7ed3757d290c3ecf2c958ee381733058ca251e1b 2755 2753 2021-11-10T15:56:19Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|350px|poster2021]] [[Media:GroupPhoto1.jpg|right|400px|groupphoto1]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. ebc9ad2138df2b1ee0d7fb8f2f5889a194440c8b 6 351 2754 2021-11-10T15:55:18Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 343 2756 2755 2021-11-10T15:56:41Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|350px|poster2021]] [[File:GroupPhoto1.jpg|right|400px|groupphoto1]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 7ed3757d290c3ecf2c958ee381733058ca251e1b 0 345 2757 2751 2021-11-10T16:59:22Z Gsawgwikiadmin 1 wikitext text/x-wiki The meeting will be accessible via Zoom to registered participants and will be streamed/recorded on YouTube for everyone else. ---- <Big>[https://docs.google.com/spreadsheets/d/1hYfoTHXGHabsx583UbzToTgj6XspoP0Azmd8A5b6plM/edit?usp=sharing Workshop Agenda on Google Spreadsheets] </Big> [[File:agenda.pdf| Agenda in PDF]] ---- Live streaming on YouTube and recordings: [https://youtu.be/9CsSaZOcPQc YouTube Monday 8 Nov 2021 14:00 EET] (note, updated link!) [https://youtu.be/vHvQB1YseP8 YouTube Tuesday 9 Nov 2021 14:00 EET] [https://youtu.be/0GVdi47pk1M YouTube Tuesday 9 Nov 2021 17:00 EET] for Bryan Holler talk [http://astrouw.edu.pl/~wyrzykow/SEM/sem211109.html Abstract] [https://youtu.be/MVsZgfmA6tk YouTube Wednesday 10 Nov 2021 15:00 EET] [https://youtu.be/Mo33p1Vtqyg YouTube Thursday 11 Nov 2021 14:00 EET] [https://youtu.be/6Hbc-W60ncc YouTube Friday 12 Nov 2021 14:00 EET] 3886d6f2ab719031ba1e5af70334b07a8f9bbd29 0 344 2758 2721 2021-11-11T11:50:25Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' --> Registration is now closed. If you want to join our online streaming please email LW at astrouw.edu.pl. ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered participants: # John Antoniadis, FORTH Institute of Astrophysics # Iair Arcavi, Tel Aviv University # Doug Arnold, Liverpool John Moores University # Etienne Bachelet, Las Cumbres Observatory # Karolina Bąkowska, N. Copernicus University # Andrea Bianco, INAF-Osservatorio Astronomico di Brera # Sumedha Biswas, Radboud University # Stephen Brincat, AAVSO # Mateusz Bronikowski, University of Nova Gorica Center for Astrophysics and Cosmology # David Buckley, SAAO # Josep Manel Carrasco, Institut de Ciències del Cosmos - Universitat de Barcelona # Arnaud Cassan, Institut d'Astrophysique de Paris # Vytautas Čepas, Vilnius university # Vassilis Charmandaris, Univ. of Crete & FORTH # Hank Corbett, University of North Carolina at Chapel Hill # Michel Dennefeld, IAP/Paris and Sorbonne University # Bob Eldering, Joint Institute for VLBI ERIC # Laurent Eyer, Geneva Observatory # Eleonora Fiorellino, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, # Octavi Fors, Institute of Cosmos Sciences (ICCUB) / IEEC # Alessia Garofalo, INAF - Osservatorio di astrofisica e scienza dello spazio di Bologna # Ilknur Gezer, Astronomical Observatory, University of Warsaw # Gerry Gilmore, Cambridge # Andreja Gomboc, University of Nova Gorica # Aleksandra Grokhovskaya, Special Astrophysical Observatory of RAS # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Tolga Guver, Istanbul University # Franz-Josef Hambsch, ROAD Observatory # Simon Hodgkin, Institute of Astronomy, Cambridge University # Kornel Howil, Astronomical Observatory, University of Warsaw # Nada Ihanec, Astronomical Observatory University of Warsaw # Maja Jabłońska, Astronomical Observatory of University of Warsaw # Helen Jermak, Astrophysics Research Institute, LJMU # Zofia Kaczmarek, Institute of Astronomy, University of Cambridge # Krzysztof Katarzyński, Institute of Astronomy NCU Poland # Adam Kawash, Michigan State University # Patrick Kelly, University of Minnesota # Sebastian Kiehlmann, Foundation of Research and Technology Hellas # Zuzanna Kostrzewa-Rutkowska, Leiden Observatory # Hariharan Krishnan, Arizona State University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Maria Kun, Konkoly Observatory, Hungary # Magdalena Kunert-Bajraszewska, Institute of Astronomy, NCU # Sebastian Kurowski, ESO Chile / Jagiellonian University # Marco Lam, Tel Aviv University # David Law, Liverpool John Moores University # Fraser Lewis, Faulkes Telescope Project # Ioannis Liodakis, Finnish Centre for Astronomy with ESO # Vladimir Lipunov, Moscow State University # Ashish Mahabal, Caltech # Gábor Marton, CSFK Konkoly Observatory # Marius Maskoliunas, Vilnius University, Institute of Theoretical Physics and Astronomy # Seppo Mattila, University of Turku # Jaroslav Merc, Astronomical Institute of Charles University # Przemysław Jan Mikołajczyk, Astronomical Institute, University of Wrocław; Astronomical Observatory, University of Warsaw # Zsofia Nagy, Konkoly Observatory (Hungary) # Marek Nikolajuk, Faculty of Physics, University of Bialystok # Waldemar Ogloza, Pedagogical Uniwersity of Cracow # Erika Pakštienė, Institute of Theoretical Physics and Astronomy at Vilnius University # Sunkyung Park, Konkoly Observatory # Gudrun Pebody, Cambridge # Tanja Petrushevska, University of Nova Gorica # Stephen Potter, South African Astronomical Observatory # Eniko Regos, Konkoly Institute of Astronomy # Kovi Rose, The Hebrew University of Jerusalem # Rupak Roy, IUCAA (In between two jobs) # Krzysztof Rybicki, Astronomical University, University of Warsaw # Elena Shablovinskaya, Special astrophysical observatory of RAS # Monika Sitek, Astronomical Observatory of Warsaw University # Patrik Sivak, Warsaw University Observatory # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Milan Stojanović, Astronomical Observatory of Belgrade # Rachel Street, Las Cumbres Observatory # Laszlo Szabados, Konkoly Observatory # Lina Tomasella, INAF Padova # Piotr Trzcionkowski, Astronomical Observatory University of Warsaw # Rūta Urbonavičiūtė, Institute of Theoretical Physics and Astronomy at Vilnius University # siegfried Vanaverbeke, astrolab IRIS observatory # Harro Verkouter, Joint Institute for VLBI ERIC # Klaas Wiersema, Lancaster University # David Williams, University of Manchester/Jodrell Bank Center for Astrophysics # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory, Poland # Justas Zdanavičius, Institute of Theoretical Physics and Astronomy, Vilnius University # Pawel Zielinski, Astronomical Observatory, University of Warsaw # Staszek Zola, Astronomical Observatory, Jagiellonian University 7713e3f1e49759b26d5e2ca818172717ad155ac2 6 325 2759 2752 2021-11-16T06:27:56Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Agenda.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 200 2760 2550 2022-04-22T15:51:12Z Gsawgwikiadmin 1 wikitext text/x-wiki The main address of the server since 2022 is: [https://cpcs.astrolabs.pl/| https://cpcs.astrolabs.pl/] The old server (http://gsaweb.ast.cam.ac.uk/followup) has been replaced with the new one listed above. == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. Updated December 2016 by LW. == Authorization == * In order to access the server you need a so called "hashtag" which is an authorization key. In order to get one you need to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the sextractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is http://gsaweb.ast.cam.ac.uk/followup You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts ). If the alert is not in our DB, you can insert it http://gsaweb.ast.cam.ac.uk/followup/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "http://gsaweb.ast.cam.ac.uk/followup/cgi/upload" Parameters of the http://gsaweb.ast.cam.ac.uk/followup/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_followups You can view the list of alerts which are in the DB http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts , and the subset of them which have followup data http://gsaweb.ast.cam.ac.uk/followup/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: http://gsaweb.ast.cam.ac.uk/followup/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org = Data Policy = If you use any of the data from the Calibration Server in your publication, please acknowledge it with the following text: '''We acknowledge the use of the Cambridge Photometric Calibration Server (http://gsaweb.ast.cam.ac.uk/followup), developed by Sergey Koposov and maintained by Lukasz Wyrzykowski, Arancha Delgado, Pawel Zielinski, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 730890 (OPTICON).''' <big>Also note that if the data from the CPCS is essential for the paper, please include the observers as co-authors.</big> 67dafb11e473f8f98b31d32e9f7761d8bc3ec660 2761 2760 2022-04-22T15:58:09Z Gsawgwikiadmin 1 wikitext text/x-wiki The main address of the server since 2022 is: [https://cpcs.astrolabs.pl/| https://cpcs.astrolabs.pl/] The old server (http://gsaweb.ast.cam.ac.uk/followup) has been replaced with the new one listed above. == The manual document == Below you can find a quick manual. For more detailed pdf version, see [http://www.astrouw.edu.pl/~wyrzykow/manualCPCS2016.pdf here]. == Authorization == In order to access the server you need a so-called "hashtag" which is an authorization key. * ''' The easiest way is to register an account in our new system, BHTOM [bhtom.space], which offers way more than the CPCS. But it also generates a hashtag for your CPCS use.''' * Alternative option (old way) is to ask Lukasz Wyrzykowski and give him also the lon,lat of your observatory and list of filters you have. * If you have the hashtag, you can use the login form of the server to authorize yourself. Or if you are doing some scripting, you will need to specify hashtag option in the GET, POST requests. == Preparing your data == In order to obtain the SExtractor file with [Ra, Dec] coordinates required by the photometric server, the following steps have to be performed. * Obtain the Equatorial coordinates for you photometry fits file by using [http://nova.astrometry.net/ Astrometry.net]. * Download the Astrometry.net output file (''new-image.fits'' by default) from the site and use it as the sextractor input. * Run sextractor: sex new-image.fits -c /path_to/default.sex * make sure SExtractor outputs those : MAG_AUTO, MAGERR_AUTO, ALPHA_J2000, DELTA_J2000 and your configuration file should state that you want the output to be ASCII file with header (CATALOG_TYPE ASCII_HEAD) * Upload the SExtractor output catalogue (by default ''test.cat'') to the Cambridge Photometry Calibration Server. == Calibration of your photometric data == The main url for calibration of your SExtractor catalogs is : [https://cpcs.astrolabs.pl/| https://cpcs.astrolabs.pl/] You first need to login with your hashtag in order to be able to upload the data and to view the observations. Without login you can still see the lightcurves of the events. ==== Data format ==== The allowed formats for the sextractor catalogs are plain ascii and FITS. We also read FITS_LDAC. The fits should have all necessary columns defined. The columns which are required (specified in ''default.params'': MAG_AUTO MAGERR_AUTO ALPHA_J2000 DELTA_J2000 If outputing as ASCII make sure the header is also outputed. Set it in ''default.sex'' as: CATALOG_TYPE ASCII_HEAD If using different photometric software than SExtractor, then please add the following header to the ASCII output: # 1 MAG_AUTO Kron-like elliptical aperture magnitude [mag] # 2 MAGERR_AUTO RMS error for AUTO magnitude [mag] # 3 ALPHA_J2000 Right ascension of barycenter (J2000) [deg] # 4 DELTA_J2000 Declination of barycenter (J2000) [deg] and make sure the columns are as described in the header (i.e. 1st is mag, 2nd is error, and so on). Also, note the separator in the data file should be space, not tab. ==== Uploading your observations ==== Before uploading, please make sure your event you have observed is on the list of alerts. You can see all alerts or only those for which there is any data already. If your event is not on the list you will need to add it manually, see below. If your event is there, then please note its ivorn (ID), because you will need to provide it while uploading the data - this helps identify the right object on your image. The upload form is straightforward. You need to provide the IVORN (the unique id of the alert), MJD of observations (note that MJD=JD-2400000.5), exposure time in seconds, optional comment on the datapoint, Sextractor catalog: browse the file here from your computer, matching radius: how accurate is your astrometry with respect to e.g. SDSS (typically 2'' is good, but you might want to try larger radii if calibration is poor). Force Filter = no (default) indicates that the filter will be determined automatically for your data - the best matching one will be used. If you know which filter is the closest to your then you can force it by choosing from the list. Dry Run: if ticked, it means this is just a test submission and nothing gets stored. You can then repeat the insertion as soon as you are happy with it. Then, switch off Dry Run and your data will get stored. Note, you will not be able to submit the same data point twice if not in Dry Run. ==== New event ==== It is important that you can upload the data for the alerts which are in the database (e.g. which are listed here https://cpcs.astrolabs.pl/list_of_alerts ). If the alert is not in our DB, you can insert it https://cpcs.astrolabs.pl/newevent/. IVORN is the unique Virtual Observatory event name, e.g. ivo://nvo.caltech/voeventnet/catot#1306271320054132125. If it is unknown the format should be, e.g. ivo://asassn/ASASSN-13ax, for ASAS-SN survey object 13ax. Ra,Dec are given in decimal degrees. URL: link to the transient's page, ideally to individual event, but if not available, then to the main page of the feeding survey, e.g. http://ogle.astrouw.edu.pl/ogle4/transients/ == Automated submission == You can also do that from the command line using HTTP POST protocol curl -F matchDist=2 -F EventID='ivo://110610' -F sexCat="@path_to_your_sex_catalog_with_filename;filename=test.cat" -F "hashtag=XXXX" -F "MJD=2" -F expTime=1 -F noPlot=1 -F forceFilter=no -F dryRun=1 -F outputFormat=json "https://cpcs.astrolabs.pl/cgi/upload" Parameters of the https://cpcs.astrolabs.pl/cgi/upload * matchDist -- matching radius in arcseconds * hashtag -- your authorization key * MJD -- mjd of the observations * expTime -- exposure time * comment -- comments * EventID -- the ivorn of the alert * dryRun -- the value of 1 allows you to check the results of the calibration without inserting anything into our DB * forceFilter -- "no" means that the calibration will be fully automated. But You can also specify APASS/V if you want to calibrate using a particular survey/filter * sexCat -- that's the Sextractor catalog you are trying to submit * outputFormat -- at the moment the only allowed values are json and html == Review of the data in the Database == You can view the list of followup_data which are in the DB https://cpcs.astrolabs.pl/list_of_followups You can view the list of alerts which are in the DB https://cpcs.astrolabs.pl/list_of_alerts , and the subset of them which have followup data https://cpcs.astrolabs.pl/list_of_alerts?observed_only=1. From these pages you can also see the light curves for those alerts which do have followup data. Here is the example of the light curve: https://cpcs.astrolabs.pl/get_alert_lc?alert_id=2999 == Source code == The calibration server is written in python using Flask framework. If you'd like to help/implement something, ask Sergey Koposov for the access to the git repository on http://bitbucket.org = Data Policy = If you use any of the data from the Calibration Server in your publication, please acknowledge it with the following text: '''We acknowledge the use of the Cambridge Photometric Calibration Server (https://cpcs.astrolabs.pl), developed by Sergey Koposov and maintained by Lukasz Wyrzykowski, Pawel Zielinski, funded by the European Union's Horizon 2020 research and innovation programme under grant agreement No 101004719 (OPTICON-RadioNET Pilot).''' <big>Also note that if the data from the CPCS is essential for the paper, please include the observers as co-authors.</big> a2e6eb0f8a6974ead446761730cbbace21b6541a 0 1 2764 2660 2022-06-28T09:58:15Z Gsawgwikiadmin 1 wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2022:main|13th ORP and Gaia Science Alerts Workshop 2022, Pula, Sardinia, 4-6 October 2022]]</Big>''' </center> ---- <center> [[Workshop2021:agenda|12th Gaia Science Alerts Workshop 2021, FORTH/Crete - archive of presentations]] [[Workshop2020:agenda|11th Gaia Science Alerts Workshop 2020, on-line - archive of presentations]] [[Workshop2019:agenda|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:agenda|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:agenda|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 8bd9dde8cda703ead403ad8c5bfeae914d9ae834 2765 2764 2022-06-28T09:58:43Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2022:main|13th ORP and Gaia Science Alerts Workshop 2022, Pula, Sardinia, 4-7 October 2022]]</Big>''' </center> ---- <center> [[Workshop2021:agenda|12th Gaia Science Alerts Workshop 2021, FORTH/Crete - archive of presentations]] [[Workshop2020:agenda|11th Gaia Science Alerts Workshop 2020, on-line - archive of presentations]] [[Workshop2019:agenda|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:agenda|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:agenda|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- 9b09919345154fbb33868ef54edf37c49e9a3333 0 352 2766 2022-06-28T10:01:11Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held Workshop2021:logis..." wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2021:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. ae47099687967daf33a61c7bd46c19604614ff5a 2768 2766 2022-07-01T16:32:14Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2021:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. f889d7cd6328b60d6f44f22f7919b16f53c75c20 2778 2768 2022-07-04T08:55:24Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2021:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. fc0c6bb2bd9e6438dfe11562d2c9c797be1cd507 2779 2778 2022-07-04T08:55:41Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2021:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. cc3018845afb481c4db47483d3080711ebbfa273 2780 2779 2022-07-04T09:25:14Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[Media:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2021:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 044a1de9bafc021fa0d28bbae5c190ba398c7dc9 2782 2780 2022-07-04T09:26:13Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2021:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. cc3018845afb481c4db47483d3080711ebbfa273 2786 2782 2022-07-08T14:10:16Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2022:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 57ca28dabb38e19bc16b16cfa67934576e4bded8 2791 2786 2022-08-27T07:28:47Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2022:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 203ec285bbd2faa1966c6a9b5940642165d70ec3 8 3 2767 2658 2022-06-28T10:03:28Z Gsawgwikiadmin 1 wikitext text/x-wiki * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys *workshop 2022 **workshop2022:main|Main Workshop Page **workshop2022:rationale|Rationale **workshop2022:agenda|Program **workshop2022:registration|Participants and Registration **workshop2022:logistics|Logistics *workshop 2021 (archive) **workshop2021:main|Main Workshop Page **workshop2021:agenda|Archive of presentations *workshop 2020 (archive) **workshop2020:main|Main Workshop Page **workshop2020:agenda|Archive of presentations *workshop 2019 (archive) **workshop2019:main|Main Workshop Page **workshop2019:agenda|Archive of presentations *workshop 2018 (archive) **workshop2018:main|Main Workshop Page **workshop2018:agenda|Archive of presentations *workshop 2017 (archive) **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 (archive) **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 (archive) **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 4b85418d1afc517d9c840ad0ce473acb28ee2e6a 0 353 2769 2022-07-01T16:40:28Z Gsawgwikiadmin 1 Created page with "=== Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of..." wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Gaia Alerts Science === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up and Time-Domain Astronomy === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. The demand for time-domain observations of transients and other time-varying astrophysical phenomena is increasing and the Opticon-Radionet Pilot (ORP) community is trying to address this with its BHTOM virtual observatory. In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 13th in the series, will be an opportunity to learn about the current state of Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia DR3 and Gaia Alerts, and we will explore the scientific potential of Gaia. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities. === Meeting in the Covid era === The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be primarily an in-person meeting and we should accommodate up to 50 attendees. You are asked in the Registration to state your preference for in-person - if we are able to host that - or on-line participation. We shall certainly host on-line participation. Given the ever-changing Covid, travel restriction and post-travel quarantine requirements, we will make a final decision on in-person participation in early-mid September. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place. d0f3c1d9ab96702a9f5505bcb5c6e30fe8377bb6 2787 2769 2022-07-08T14:12:53Z Gsawgwikiadmin 1 /* Gaia Alerts Science */ wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Science with Gaia Alerts === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up and Time-Domain Astronomy === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. The demand for time-domain observations of transients and other time-varying astrophysical phenomena is increasing and the Opticon-Radionet Pilot (ORP) community is trying to address this with its BHTOM virtual observatory. In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 13th in the series, will be an opportunity to learn about the current state of Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia DR3 and Gaia Alerts, and we will explore the scientific potential of Gaia. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities. === Meeting in the Covid era === The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be primarily an in-person meeting and we should accommodate up to 50 attendees. You are asked in the Registration to state your preference for in-person - if we are able to host that - or on-line participation. We shall certainly host on-line participation. Given the ever-changing Covid, travel restriction and post-travel quarantine requirements, we will make a final decision on in-person participation in early-mid September. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place. 64498e5eb66e28948ff9a1b83fdb9e501205af1f 2788 2787 2022-07-08T14:13:02Z Gsawgwikiadmin 1 /* Follow-up and Time-Domain Astronomy */ wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Science with Gaia Alerts === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up and Time-Domain Astronomy === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. The demand for time-domain observations of transients and other time-varying astrophysical phenomena is increasing and the Opticon-Radionet Pilot (ORP) community is trying to address this with its BHTOM virtual observatory. In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 13th in the series, will be an opportunity to learn about the current state of Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia DR3 and Gaia Alerts, and we will explore the scientific potential of Gaia. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities. === Meeting in the Covid era === The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be primarily an in-person meeting and we should accommodate up to 50 attendees. You are asked in the Registration to state your preference for in-person - if we are able to host that - or on-line participation. We shall certainly host on-line participation. Given the ever-changing Covid, travel restriction and post-travel quarantine requirements, we will make a final decision on in-person participation in early-mid September. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place. 8b4d7a43133ee662b9894ca35873e45a82f04992 2789 2788 2022-07-08T14:14:24Z Gsawgwikiadmin 1 /* Meeting in the Covid era */ wikitext text/x-wiki === Gaia and Gaia Alerts === ESA Gaia is continuing operations and is now well into its extended mission. In June 2022 Gaia consortium has released DR3 with a huge wealth of data products, including unprecedented astrometric, photometric and spectroscopic data. In the meantime, Gaia Photometric Science Alerts system continues its operation as a well established and leading transient survey. It discovers nearly 4000 objects a year from all over the sky, down to G=19, covering all possible classes of transients, from supernovae and CVs to rare phenomena like microlensing events or pair-instability supernovae. === Science with Gaia Alerts === 
 The transient discovery machine within Gaia is constantly evolving allowing for more accurate transient identification. The longer baseline of Gaia data also allows for more robust detections of photometric anomalies. The alerting system is now also sensitive to slowly changing astrophysical events such as flares in distant quasars, young stellar objects, Be-type stars and microlensing events due to massive lenses. 
 === Follow-up and Time-Domain Astronomy === At the same time, we are seeing significant evolution in the area of photometric and spectroscopic follow-up. Robotisation and queue-scheduling of many telescopes enables more efficient coordination of long-term time-domain observations. The demand for time-domain observations of transients and other time-varying astrophysical phenomena is increasing and the Opticon-Radionet Pilot (ORP) community is trying to address this with its BHTOM virtual observatory. In particular, for this workshop we would like to extend the invitation to all time-domain astronomical activities, spanning all electromagnetic spectrum from radio, through optical to X-rays, and other domains (gravitational waves, neutrino detectors). We hope this workshop will be an opportunity for improving the coordination within time-domain astronomy and increasing the scientific output of surveys and follow-up observations in the multi-messenger era. === Workshop's promise === 
 The forthcoming Gaia Alerts Workshop, the 13th in the series, will be an opportunity to learn about the current state of Gaia and Gaia Alerts. We aim to discuss the detection, filtering, classification and publication of candidates. We will discover the most recent scientific highlights from Gaia DR3 and Gaia Alerts, and we will explore the scientific potential of Gaia. During the workshop we will also explore the new possibilities offered by the Opticon-Radionet-Pilot H2020 in planning, obtaining and reducing in an efficient manner follow-up observations of transient alerts reported by other (non-GAIA) facilities. === Meeting in the Covid era === The successful experience of our previous meetings shows that working personal interactions are highly effective at developing plans, solving challenges, and extending partnerships to new participants. For that reason, we hope this can be primarily an in-person meeting and we should accommodate up to 50 attendees. You are asked in the Registration to state your preference for in-person - if we are able to host that - or online participation. We shall certainly host online participation. Given the ever-changing Covid, travel restrictions and post-travel quarantine requirements, we will make a final decision on in-person participation in early September. Individuals should follow their national guidance. For travel organising, please do ensure you have full cancellation and health cover insurance in place. 6af1403fe5f6c09d0eb1d966479576e589b9c40e 0 354 2770 2022-07-02T08:02:55Z Gsawgwikiadmin 1 Created page with "= Workshop venue The Workshop will be held in Sardinia (Italy) in the [https://www.hotelbaiadinora.com/ | Baia di Nora hotel] in Pula, 40 km South from Cagliari. The worksho..." wikitext text/x-wiki = Workshop venue The Workshop will be held in Sardinia (Italy) in the [https://www.hotelbaiadinora.com/ | Baia di Nora hotel] in Pula, 40 km South from Cagliari. The workshop will be held in a dedicated conference room which holds 50 inside the hotel. Lunch and coffee breaks will be served in the same hotel and will be covered by the organisers for the first three days of the workshop. The last of the workshop is expected to have an informal format. = Transport A shuttle service with minibus or private car will be available from/to Airport and has to be requested directly to the hotel. Every 40 minutes is also available a public bus (Line 129) that starts in Pula’s center (1,8 km / 23 mins by foot from the hotel) that arrives in Cagliari center in 1h 15min. If needed, once in Cagliari, there is a train from the station to the airport. = Accommodation The hotel is located on a beach with transparent sea and disposes of all types of comforts like swimming pool, training area, spa, parks for kids, bike rental and so on. Please visit the webpage to get more information: Here the form to ask for a service in English: https://www.hotelbaiadinora.com/en/check-availability/ We strongly recommended to book a room at the same hotel during the workshop. We already agreed some discount for our group. = Extra During the meeting we foresee a visit to the Sardinia Radio Telescope, most likely on Friday, further details will be communicated soon here and on the program page. It will be possible to visit the Nora ruins directly by foot from the hotel (1.5 km of distance). = Social dinner Planned for Thursday evening. Venue to be decided. 213849b4143051f070e02b6ed2f010e5ed81dffc 2771 2770 2022-07-02T08:03:14Z Gsawgwikiadmin 1 wikitext text/x-wiki = Workshop venue = The Workshop will be held in Sardinia (Italy) in the [https://www.hotelbaiadinora.com/ | Baia di Nora hotel] in Pula, 40 km South from Cagliari. The workshop will be held in a dedicated conference room which holds 50 inside the hotel. Lunch and coffee breaks will be served in the same hotel and will be covered by the organisers for the first three days of the workshop. The last of the workshop is expected to have an informal format. = Transport = A shuttle service with minibus or private car will be available from/to Airport and has to be requested directly to the hotel. Every 40 minutes is also available a public bus (Line 129) that starts in Pula’s center (1,8 km / 23 mins by foot from the hotel) that arrives in Cagliari center in 1h 15min. If needed, once in Cagliari, there is a train from the station to the airport. = Accommodation = The hotel is located on a beach with transparent sea and disposes of all types of comforts like swimming pool, training area, spa, parks for kids, bike rental and so on. Please visit the webpage to get more information: Here the form to ask for a service in English: https://www.hotelbaiadinora.com/en/check-availability/ We strongly recommended to book a room at the same hotel during the workshop. We already agreed some discount for our group. = Extra = During the meeting we foresee a visit to the Sardinia Radio Telescope, most likely on Friday, further details will be communicated soon here and on the program page. It will be possible to visit the Nora ruins directly by foot from the hotel (1.5 km of distance). = Social dinner = Planned for Thursday evening. Venue to be decided. 4d75071a7c576aebe2d1723024c39d4966838854 2772 2771 2022-07-02T08:03:35Z Gsawgwikiadmin 1 wikitext text/x-wiki = Workshop venue = The Workshop will be held in Sardinia (Italy) in the [https://www.hotelbaiadinora.com/ Baia di Nora hotel] in Pula, 40 km South from Cagliari. The workshop will be held in a dedicated conference room which holds 50 inside the hotel. Lunch and coffee breaks will be served in the same hotel and will be covered by the organisers for the first three days of the workshop. The last of the workshop is expected to have an informal format. = Transport = A shuttle service with minibus or private car will be available from/to Airport and has to be requested directly to the hotel. Every 40 minutes is also available a public bus (Line 129) that starts in Pula’s center (1,8 km / 23 mins by foot from the hotel) that arrives in Cagliari center in 1h 15min. If needed, once in Cagliari, there is a train from the station to the airport. = Accommodation = The hotel is located on a beach with transparent sea and disposes of all types of comforts like swimming pool, training area, spa, parks for kids, bike rental and so on. Please visit the webpage to get more information: Here the form to ask for a service in English: https://www.hotelbaiadinora.com/en/check-availability/ We strongly recommended to book a room at the same hotel during the workshop. We already agreed some discount for our group. = Extra = During the meeting we foresee a visit to the Sardinia Radio Telescope, most likely on Friday, further details will be communicated soon here and on the program page. It will be possible to visit the Nora ruins directly by foot from the hotel (1.5 km of distance). = Social dinner = Planned for Thursday evening. Venue to be decided. 8a30933060f54cfcca89740b17cb534eba3cfc4b 0 355 2773 2022-07-02T13:24:44Z Gsawgwikiadmin 1 Created page with "Very drafty plan: Tue, 4.Oct.2022, from 9:00: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 9:00: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 9:00..." wikitext text/x-wiki Very drafty plan: Tue, 4.Oct.2022, from 9:00: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 9:00: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 9:00: Day 3, conference room in the hotel, Conference Dinner Fri, 7.Oct.2022, informal meetings day, individual meetings, technical support consultations, trip to the radiotelescope. 640973c3f8b2d9addd9505d6a36d5a2c2b7928a9 2790 2773 2022-08-27T07:28:17Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will consist of talks proposed by the attendees. Very drafty plan: Tue, 4.Oct.2022, from 9:00: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 9:00: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 9:00: Day 3, conference room in the hotel, Conference Dinner Fri, 7.Oct.2022, individual and subgroups meetings, technical support consultations, trip to the radiotelescope. 6ff9e0f8894aa2f3b572a31e99da1d9e35b1b9a8 2799 2790 2022-09-11T09:10:41Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will consist of talks proposed by the attendees. Very drafty plan: Tue, 4.Oct.2022, from 9:00: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 9:00: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 9:00: Day 3, conference room in the hotel, Conference Dinner Fri, 7.Oct.2022, individual and subgroups meetings, technical support consultations, trip to the radiotelescope (or Sat). --- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On Saturday, 8th of October, individual consultations are also possible and the trip to the observatory is planned. e3df99f433fe63d3b2a3f89e1e2493a0d9079427 2800 2799 2022-09-11T09:10:49Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will consist of talks proposed by the attendees. Very drafty plan: Tue, 4.Oct.2022, from 9:00: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 9:00: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 9:00: Day 3, conference room in the hotel, Conference Dinner Fri, 7.Oct.2022, individual and subgroups meetings, technical support consultations, trip to the radiotelescope (or Sat). ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On Saturday, 8th of October, individual consultations are also possible and the trip to the observatory is planned. 8e9db0fceb7356086f9ee371d2b2347deac7c3e8 2801 2800 2022-09-11T09:10:58Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will consist of talks proposed by the attendees. Very drafty plan: Tue, 4.Oct.2022, from 9:00: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 9:00: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 9:00: Day 3, conference room in the hotel, Conference Dinner Fri, 7.Oct.2022, individual and subgroups meetings, technical support consultations, trip to the radiotelescope (or Sat). ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On Saturday, 8th of October, individual consultations are also possible and the trip to the observatory is planned. a4544e41a04a09d9ea7c47d0ccffd3f7ec4a28b7 2804 2801 2022-09-24T21:17:04Z Gsawgwikiadmin 1 wikitext text/x-wiki The programme will consist of talks proposed by the attendees. Very draft plan: Tue, 4.Oct.2022, from 9:30: Day 1, conference room in the hotel Wed, 5.Oct.2022, from 10:30: Day 2, conference room in the hotel Thu, 6.Oct.2022, from 10:30: Day 3, conference room in the hotel, Conference Dinner Fri, 7.Oct.2022, individual and subgroups meetings, technical support consultations, trip to the radiotelescope (or Sat). ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On Saturday, 8th of October, individual consultations are also possible and the trip to the observatory is planned. 5f2d099eb84f044238fdc11cd94923fc9eb9394b 2806 2804 2022-09-26T15:08:17Z Gsawgwikiadmin 1 wikitext text/x-wiki The Workshop's agenda is available as a [https://docs.google.com/spreadsheets/d/1hL1KkbvD249RxC_yVhMRybRexOgC0aXQq8ptQaEwfK0/edit?usp=sharing Google Spreadsheet here]. ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On Saturday, 8th of October, individual consultations are also possible and the trip to the observatory is planned (or on Friday). 0f8120cd6f1dc8f3f355635896962fd97d210be7 2807 2806 2022-09-26T15:08:59Z Gsawgwikiadmin 1 wikitext text/x-wiki <Big> '''The Workshop's agenda is available as a [https://docs.google.com/spreadsheets/d/1hL1KkbvD249RxC_yVhMRybRexOgC0aXQq8ptQaEwfK0/edit?usp=sharing Google Spreadsheet here].</Big>''' ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On Saturday, 8th of October, individual consultations are also possible and the trip to the observatory is planned (or on Friday). 210f494c851edd2a7fe458b8f55a9369997baa1d 0 356 2774 2022-07-02T13:29:17Z Gsawgwikiadmin 1 Created page with "<!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> —-> The registration opens soon. We can only accommodate 50 attendees on-s..." wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> —-> The registration opens soon. We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. ‘’’There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again.’’’ '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' 43c7263b5321afd8cd3176fd38fb0031e1def64a 2775 2774 2022-07-02T13:29:52Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/6vfzPbcPDumNhWeK8 Registration is OPEN until 15.October]'''</big> —-!> The registration opens soon. We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. ‘’’There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again.’’’ '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' 04e24031903d407d9ed18e284d17a09672069467 2776 2775 2022-07-02T13:30:17Z Gsawgwikiadmin 1 wikitext text/x-wiki The registration opens soon. We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. ‘’’There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again.’’’ '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' bf718bdb558f07e2f1cb0f90df2f4e64cbe50a02 2777 2776 2022-07-02T13:30:46Z Gsawgwikiadmin 1 wikitext text/x-wiki The registration opens soon. We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' a7628995fdfe682a746614c49019a3b9563331fa 2784 2777 2022-07-08T10:21:05Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' cb0df07b18cd180a491964eed63675c988e80642 2785 2784 2022-07-08T10:28:06Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- 2cac0a09f36a12697a07b94d18b2b7fa43ab9905 2792 2785 2022-09-08T08:34:16Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl. ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- eed5be281dadb58438bc2494148dd41de8fd46ac 2793 2792 2022-09-08T08:34:32Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- d2334fe999c01bf7d90d8babe5c8b47a6fdd3e48 2794 2793 2022-09-08T08:53:36Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation). Please clearly state your preference in the registration form.''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- ''There is a very limited possibility for financial support for travel if the meeting takes place physically. Please get in touch with lw at astrouw.edu.pl with your request and justification, including the proposed budget.'' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy , Shahjalal University of Science and Technology # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences f44562f5061de5de8000f6fc06c67ddefc2b254c 2795 2794 2022-09-08T10:28:33Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy , Shahjalal University of Science and Technology # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 1feef38362a30afb005e1de18db43c883200d4c7 2796 2795 2022-09-08T22:30:40Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Kornel Howil, Warsaw University Astronomical Observatory # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy , Shahjalal University of Science and Technology # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 120078f8f59e696e431858ed0da276f5061ad0aa 2797 2796 2022-09-09T15:15:48Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Kornel Howil, Warsaw University Astronomical Observatory # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy , Shahjalal University of Science and Technology # Tanja Petrushevska, University of Nova Gorica, Slovenia # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences a693bd9663c552f6f3bafafdb11f60dca2dda0aa 2798 2797 2022-09-11T08:58:31Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF (invited) # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge (invited) # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Kornel Howil, Warsaw University Astronomical Observatory # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University (invited) # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy, Shahjalal University of Science and Technology # Tanja Petrushevska, University of Nova Gorica, Slovenia (invited) # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences aa2468d48f671e1dce229e9b716025789948fd34 2802 2798 2022-09-15T11:23:21Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF (invited) # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge (invited) # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Kornel Howil, Warsaw University Astronomical Observatory # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marcin Gawroński, Institute of Astronomy, Nicolaus Copernicus University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University (invited) # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy, Shahjalal University of Science and Technology # Tanja Petrushevska, University of Nova Gorica, Slovenia (invited) # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences b11b332aba89d8c5b87ba321d6303d530c74675b 2803 2802 2022-09-16T10:22:10Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF (invited) # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge (invited) # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jakob Nordin, Humboldt University of Berlin # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Krzysztof Rybicki, Weizmann Institute of Science # Kornel Howil, Warsaw University Astronomical Observatory # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marco Lam, Tel Aviv University # Marcin Gawroński, Institute of Astronomy, Nicolaus Copernicus University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University (invited) # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy, Shahjalal University of Science and Technology # Tanja Petrushevska, University of Nova Gorica, Slovenia (invited) # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 042f1fd22f64d094a63ce0e987f2a1c29ffe9e72 2805 2803 2022-09-26T09:44:33Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jakob Nordin, Humboldt University of Berlin # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Kornel Howil, Astronomical Observatory, University of Warsaw # Krzysztof Rybicki, Weizmann Institute of Science # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marcin Gawroński, Institute of Astronomy, Nicolaus Copernicus University # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milan Stojanovic, Astronomical Observatory of Belgrade # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Piotr Kolenderski, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy , Shahjalal University of Science and Technology # Tanja Petrushevska, University of Nova Gorica, Slovenia # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 1659fe12c2b7ed36ab62c01f0fb4bd086d439ede 6 357 2781 2022-07-04T09:25:51Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 358 2783 2022-07-04T09:29:55Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 355 2808 2807 2022-09-30T13:35:44Z Gsawgwikiadmin 1 wikitext text/x-wiki <Big> '''The Workshop's agenda is available as a [https://docs.google.com/spreadsheets/d/1hL1KkbvD249RxC_yVhMRybRexOgC0aXQq8ptQaEwfK0/edit?usp=sharing Google Spreadsheet here].</Big>''' ---- YouTube Streaming from the plenary sessions (4-6.Oct): * [https://youtu.be/hJOSLCbnVXM Tuesday 4.Oct.2022, morning session, 9:30-13:00] * [https://youtu.be/VpAOR_nn2ic Tuesday 4.Oct.2022, afternoon session, 14:30-17:30] * [https://youtu.be/KyZYOLKSth4 Wednesday 5.Oct.2022, morning session, 9:00-13:00] * [https://youtu.be/ACnkfzsP6pQ Wednesday 5.Oct.2022, afternoon session, 14:30-18:30] * [https://youtu.be/WJbvcb10nag Thursday 6.Oct.2022, morning session, 9:30-13:00] * [https://youtu.be/HRVbzIn47Cw Thursday 6.Oct.2022, afternoon session, 14:30-15:30] ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On 7th and 8th of October, individual consultations are also possible and the trip to the observatory is planned. 9d9dd0353ff014835dfdfbe71dd03aa6593711f1 2811 2808 2022-10-03T16:36:57Z Gsawgwikiadmin 1 wikitext text/x-wiki <Big> '''The Workshop's agenda is available as a [https://docs.google.com/spreadsheets/d/1hL1KkbvD249RxC_yVhMRybRexOgC0aXQq8ptQaEwfK0/edit?usp=sharing Google Spreadsheet here].</Big>''' ---- YouTube Streaming from the plenary sessions (4-6.Oct): * [https://youtu.be/hJOSLCbnVXM Tuesday 4.Oct.2022, morning session, 9:30-13:00] * [https://youtu.be/SKsiCWiSyFY Tuesday 4.Oct.2022, afternoon session, 14:30-17:30] * [https://youtu.be/KyZYOLKSth4 Wednesday 5.Oct.2022, morning session, 9:00-13:00] * [https://youtu.be/ACnkfzsP6pQ Wednesday 5.Oct.2022, afternoon session, 14:30-18:30] * [https://youtu.be/WJbvcb10nag Thursday 6.Oct.2022, morning session, 9:30-13:00] * [https://youtu.be/HRVbzIn47Cw Thursday 6.Oct.2022, afternoon session, 14:30-15:30] ---- On Monday, 3rd of October, there will be an internal DAINA grant meeting in Pula. On 7th and 8th of October, individual consultations are also possible and the trip to the observatory is planned. 10df3a54785088c5c95de427bb0287742620d15a 0 354 2809 2772 2022-10-02T14:31:25Z Gsawgwikiadmin 1 wikitext text/x-wiki = Workshop venue = The Workshop will be held in Sardinia (Italy) in the [https://www.hotelbaiadinora.com/ Baia di Nora hotel] in Pula, 40 km South from Cagliari. The workshop will be held in a dedicated conference room which holds 50 inside the hotel. Lunch and coffee breaks will be served in the same hotel and will be covered by the organisers for the first three days of the workshop. The last of the workshop is expected to have an informal format. = Transport = A shuttle service with minibus or private car will be available from/to Airport and has to be requested directly to the hotel. Every 40 minutes is also available a public bus (Line 129) that starts in Pula’s center (1,8 km / 23 mins by foot from the hotel) that arrives in Cagliari center in 1h 15min. If needed, once in Cagliari, there is a train from the station to the airport. = Accommodation = The hotel is located on a beach with transparent sea and disposes of all types of comforts like swimming pool, training area, spa, parks for kids, bike rental and so on. Please visit the webpage to get more information: Here the form to ask for a service in English: https://www.hotelbaiadinora.com/en/check-availability/ We strongly recommended to book a room at the same hotel during the workshop. We already agreed some discount for our group. = Extra = During the meeting we foresee a visit to the Sardinia Radio Telescope, most likely on Friday, further details will be communicated soon here and on the program page. It will be possible to visit the Nora ruins directly by foot from the hotel (1.5 km of distance). = Social dinner = Planned for Thursday evening 19:30 in the hotel's restaurant. = Restaurants in Pula = Recommended restaurants nearby [https://www.tripadvisor.it/Restaurant_Review-g194870-d17652604-Reviews-Locanda_Caddeo_Pula-Pula_Province_of_Cagliari_Sardinia.html Locanda Caddeo] [https://www.tripadvisor.it/Restaurant_Review-g194870-d12341953-Reviews-Agriturismo_Sa_Prantaxia-Pula_Province_of_Cagliari_Sardinia.html Agriturismo Sa Prantaxia] [https://www.tripadvisor.it/Restaurant_Review-g194870-d3345775-Reviews-Fradis_Minoris-Pula_Province_of_Cagliari_Sardinia.html Fradis Minoris ($$$$$)] [https://www.tripadvisor.it/Restaurant_Review-g194870-d23961624-Reviews-Sa_Domu_Sarda_Pula-Pula_Province_of_Cagliari_Sardinia.html Sa Domu Sarda Pula] ddcee8507c6035b998ff2901803f1d947389a971 2810 2809 2022-10-02T14:32:02Z Gsawgwikiadmin 1 /* Extra */ wikitext text/x-wiki = Workshop venue = The Workshop will be held in Sardinia (Italy) in the [https://www.hotelbaiadinora.com/ Baia di Nora hotel] in Pula, 40 km South from Cagliari. The workshop will be held in a dedicated conference room which holds 50 inside the hotel. Lunch and coffee breaks will be served in the same hotel and will be covered by the organisers for the first three days of the workshop. The last of the workshop is expected to have an informal format. = Transport = A shuttle service with minibus or private car will be available from/to Airport and has to be requested directly to the hotel. Every 40 minutes is also available a public bus (Line 129) that starts in Pula’s center (1,8 km / 23 mins by foot from the hotel) that arrives in Cagliari center in 1h 15min. If needed, once in Cagliari, there is a train from the station to the airport. = Accommodation = The hotel is located on a beach with transparent sea and disposes of all types of comforts like swimming pool, training area, spa, parks for kids, bike rental and so on. Please visit the webpage to get more information: Here the form to ask for a service in English: https://www.hotelbaiadinora.com/en/check-availability/ We strongly recommended to book a room at the same hotel during the workshop. We already agreed some discount for our group. = Extra = During the meeting we foresee a visit to the Sardinia Radio Telescope on Friday. It will be possible to visit the Nora ruins directly by foot from the hotel (1.5 km of distance). = Social dinner = Planned for Thursday evening 19:30 in the hotel's restaurant. = Restaurants in Pula = Recommended restaurants nearby [https://www.tripadvisor.it/Restaurant_Review-g194870-d17652604-Reviews-Locanda_Caddeo_Pula-Pula_Province_of_Cagliari_Sardinia.html Locanda Caddeo] [https://www.tripadvisor.it/Restaurant_Review-g194870-d12341953-Reviews-Agriturismo_Sa_Prantaxia-Pula_Province_of_Cagliari_Sardinia.html Agriturismo Sa Prantaxia] [https://www.tripadvisor.it/Restaurant_Review-g194870-d3345775-Reviews-Fradis_Minoris-Pula_Province_of_Cagliari_Sardinia.html Fradis Minoris ($$$$$)] [https://www.tripadvisor.it/Restaurant_Review-g194870-d23961624-Reviews-Sa_Domu_Sarda_Pula-Pula_Province_of_Cagliari_Sardinia.html Sa Domu Sarda Pula] 741fee842645eb193bddb3535616419db9498b56 0 356 2812 2805 2022-11-10T07:57:05Z Gsawgwikiadmin 1 wikitext text/x-wiki <!-- <big>'''[https://forms.gle/b7L6tNKHxbu2tdDKA Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' --> '''The registration is now closed. In case you still want to join us, please email lw AT astrouw.edu.pl.''' ---- Please note that due to the uncertain global situation with the Covid-19 pandemic, we reserve the right to cancel the event and move it entirely to the on-line. ---- List of registered attendees: # Agnieszka Słowikowska, Nicolaus Copernicus University in Toruń # Algita Stankevičiūtė, Astronomical Observatory of the University of Warsaw # Bartosz Kirpluk, The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. # Charles Galdies , University of Malta # Elmé Breedt, Institute of Astronomy, University of Cambridge # Emilio Molinari, INAF # Etienne Bachelet, Institut d'Astrophysique de Paris # Fatma TEZCAN, Atatürk University # Franz-Josef Hambsch, ROAD Observatory # Gerry Gilmore, IoA Cambridge - invited # Giuseppe Morello, IAC # Gudrun Pebody, IoA University of Cambridge # Hai-Feng , Rome Fermi center and Rome Univ. # Himanshu Verma , Indian Institute of Technology, Bombay, India # Jakob Nordin, Humboldt University of Berlin # Jaroslav Merc, Astronomical Institute of Charles University # JOHN MORA, Inter-University Centre for Astronomy and Astrophysics (IUCAA) # Karolina Bąkowska, Nicolaus Copernicus University # Katarzyna Kruszyńska, Astronomical Observatory, University of Warsaw # Klaas Wiersema, Lancaster University # Kornel Howil, Astronomical Observatory, University of Warsaw # Krzysztof Rybicki, Weizmann Institute of Science # Laszlo Szabados, Konkoly Observatory # Lukasz Wyrzykowski, Warsaw University Astronomical Observatory # Maja Jabłońska, University of Warsaw # Marcin Gawroński, Institute of Astronomy, Nicolaus Copernicus University # Marco Lam, Tel Aviv University # Marius Maskoliunas, Institute of Theoretical Physics and Astronomy, Vilnius University # Mariusz Gromadzki, Astronomical Observatory, University of Warsaw # Mateusz Motyliński, Nicolaus Copernicus University in Toruń # Michael Smith, University of Kent # Michal Zejmo, Janusz Gil Institute of Astronomy of the University of Zielona Gora # Michel Dennefeld, IAP/Paris and Sorbonne Universities # Milan Stojanovic, Astronomical Observatory of Belgrade # Milena Ratajczak, Astronomical Observatory, University of Warsaw # Monika Sitek, Astronomical Observatory of Warsaw University # Nada Ihanec, Astronomical Observatory, University of Warsaw, and ESO, Chile # Paolo Rota, Università degli Studi di Salerno # Patrik Sivak, Astronomical University Warsaw # Pawel Zielinski, Institute of Astronomy, Nicolaus Copernicus University in Torun # Piotr Kolenderski, Nicolaus Copernicus University in Torun # Przemysław J. Mikołajczyk, Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wrocław # Rachel Street, Las Cumbres Observatory - invited # Rupak Roy, Manipal Centre for Natural Sciences (MCNS), Manipal Academy of Higher Education (MAHE) # Sarang Shah, Indian Institute of Astrophysics # Silvia Pietroni, UNISA # Simon Hodgkin, IoA, Cambridge University # Somayeh Khakpash, Rutgers University # Staszek Zola, Jagiellonian University # Stephane Basa, Laboratoire d'Astrophysique de Marseille # Stephen Brincat, AAVSO # Sumit Roy Pronoy , Shahjalal University of Science and Technology # Tanja Petrushevska, University of Nova Gorica, Slovenia - invited # Teimuraz Kvernadze, Georgian National Astrophysical Observatory # Thierry Midavaine, SAF # Uliana Pylypenko, Astronomical Observatory of the University of Warsaw # Valerio Bozza, Università di Salerno # Vira Godunova, ICAMER Observatory of NAS of Ukraine # Vytautas Čepas, Vilnius university # William Thuillot, Paris Observatory # Zofia Kaczmarek, University of Cambridge / MPIA Heidelberg # Zsófia Nagy, Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 86b3e7c4fe71dc96d2ffe259772533e344545a38 0 352 2813 2791 2023-04-12T10:21:39Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2022-small.png|right|350px|poster2022]] '''The 13th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2022:logistics | in Pula, at the island of Sardinia, Italy, and online 4-7 October 2022]]''' The main goals of the workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2022:rationale|Rationale]] * [[workshop2022:agenda|Agenda]] * [[workshop2022:registration|Registration]] * [[workshop2022:logistics|Logistical information]] * [[Media:Poster2022.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Emilio Molinari (Cagliari) * Paolo Soletta (Cagliari) * Rob Beswick (Manchester) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) * Nada Ihanec (Warsaw/ESO) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. e0d89fa01fcc4b61f81ac8b9e8222ce4a9271a9a 0 343 2814 2756 2023-04-12T10:22:30Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2021-small.png|right|350px|poster2021]] [[File:GroupPhoto1.jpg|right|400px|groupphoto1]] '''The 12th Gaia Science Alerts workshop and the First ORP Time-Domain meeting will be held at the premises of the [[Workshop2021:logistics | Institute of Astrophysics-FORTH at the island of Crete, Greece, and online 8-12 November 2021]]''' The main goals of this year's workshop are: * update on the Gaia mission * update on the improvements in the Gaia Alerts * Gaia Alerts highlights and results * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * new photometric calibration server * organization of the follow-up ---- * [[workshop2021:rationale|Rationale]] * [[workshop2021:agenda|Agenda]] * [[workshop2021:registration|Registration]] * [[workshop2021:logistics|Logistical information]] * [[Media:Poster2021.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Vassilis Charmandaris (FORTH) * Simon Hodgkin (Cambridge) * Rob Beswick (Manchester) * Kasia Kruszynska (Warsaw) * Gerry Gilmore (Cambridge) * Marius Maskoliunas (Vilnius) * Nada Ihanec (Warsaw/ING) The workshop is supported jointly by the EC H2020 ORP grant no 101004719, Polish NCN DAINA grant No. 2017/27/L/ST9/03221 and Lithuanian RC DAINA grant No. S-LL-19-2. 76fd1571f5d9ffe40a177f4716f9835ff34cd729 0 1 2815 2765 2023-05-15T13:22:35Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2023:main|14th ORP and Gaia Science Alerts Workshop 2023, Valetta, Malta, 2-5 October 2023]]</Big>''' </center> ---- <center> [[Workshop2022:agenda|13th ORP and Gaia Science Alerts Workshop 2022, Pula, Sardinia, 4-7 October 2022]] [[Workshop2021:agenda|12th Gaia Science Alerts Workshop 2021, FORTH/Crete - archive of presentations]] [[Workshop2020:agenda|11th Gaia Science Alerts Workshop 2020, on-line - archive of presentations]] [[Workshop2019:agenda|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:agenda|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:agenda|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- d513e10a486709499361fb640c9bf5bf708c3f22 2817 2815 2023-05-15T13:25:15Z Gsawgwikiadmin 1 /* Workshops */ wikitext text/x-wiki = '''Welcome to the web site of the Gaia Science Alerts Working Group!''' = The Gaia Science Alerts Working Group is focussed on the real-time detection of variable sources. These include supernovae, microlensing events, exploding and eruptive stars, etc. ---- == Workshops == <center> '''<Big>[[Workshop2023:main|14th ORP and Gaia Science Alerts Workshop 2023, Valetta, Malta, 2-5 October 2023]]</Big>''' </center> ---- <center> [[Workshop2022:agenda|13th ORP and Gaia Science Alerts Workshop 2022, Pula/Sardinia - archive of presentation]] [[Workshop2021:agenda|12th Gaia Science Alerts Workshop 2021, FORTH/Crete - archive of presentations]] [[Workshop2020:agenda|11th Gaia Science Alerts Workshop 2020, on-line - archive of presentations]] [[Workshop2019:agenda|10th Gaia Science Alerts Workshop 2019, Catania - archive of presentations]] [[Workshop2018:agenda|9th Gaia Science Alerts Workshop 2018, Vipava - archive of presentations]] [[Workshop2017:agenda|8th Gaia Science Alerts Workshop 2017, Warsaw - archive of presentations]] [[Workshop2016:agenda|7th Gaia Science Alerts Workshop 2016, Utrecht - archive of presentations]] [[Workshop2015:agenda|6th Gaia Science Alerts Workshop 2015, Liverpool - archive of presentations]] [[Workshop2014:agenda|5th Gaia Science Alerts Workshop 2014, Warsaw - archive of presentations]] [[Workshop2013:agenda|4th Gaia Science Alerts Workshop 2013, Paris - archive of presentations]] [[Workshop2012:agenda|Gaia Science Alerts Workshop 2012, Bologna - archive of presentations]] [[Workshop2011:agenda|Gaia Science Alerts Workshop 2011, Cambridge - archive of presentations]] [[Workshop2010:agenda|Gaia Science Alerts Workshop 2010, Cambridge - archive of presentations]] </center> ---- '''The pages can be viewed without any restrictions. In order to add or edit them you need a password. Contact the administrator for personalized account.''' ---- ''This wiki is maintained by [[user:lukasz|Lukasz Wyrzykowski]]. '' ---- e87897b2ccd257c7d9df079f0cbbcc4a279a92d8 8 3 2816 2767 2023-05-15T13:24:24Z Gsawgwikiadmin 1 wikitext text/x-wiki *workshop 2023 **workshop2023:main|Main Workshop Page **workshop2023:rationale|Rationale **workshop2023:agenda|Program **workshop2023:registration|Participants and Registration **workshop2023:logistics|Logistics *workshop 2022 (archive) **workshop2022:main|Main Workshop Page **workshop2022:agenda|Archive of presentations *workshop 2021 (archive) **workshop2021:main|Main Workshop Page **workshop2021:agenda|Archive of presentations *workshop 2020 (archive) **workshop2020:main|Main Workshop Page **workshop2020:agenda|Archive of presentations *workshop 2019 (archive) **workshop2019:main|Main Workshop Page **workshop2019:agenda|Archive of presentations *workshop 2018 (archive) **workshop2018:main|Main Workshop Page **workshop2018:agenda|Archive of presentations *workshop 2017 (archive) **workshop2017:main|Main Workshop Page **workshop2017:agenda|Archive of presentations *workshop 2016 (archive) **workshop2016:main|Main Workshop Page **workshop2016:agenda|Archive of presentations *workshop 2015 (archive) **workshop2015:main|Main Workshop Page **workshop2015:agenda|Archive of presentations *workshop 2014 (archive) **workshop2014:main|Main Workshop Page **workshop2014:agenda|Archive of presentations * workshop 2013 (archive) ** workshop2013:main|Main Workshop Page ** workshop2013:agenda|Archive of presentations * workshop 2012 (archive) ** workshop2012:main|Main Workshop Page ** workshop2012:agenda|Archive of presentations * workshop 2011 (archive) ** workshop2011:main|Main Workshop Page ** workshop2011:agenda|Archive of presentations * workshop 2010 (archive) ** workshop2010:main|Main Workshop Page ** workshop2010:agenda|Archive of presentations * GSA Working Group ** mainpage|mainpage-description ** working groups|Working Groups * Science ** triggers|Triggers ** contaminants|Contaminants * Alerts ** detection system|Detection System ** Verification phase|Verification phase ** follow-up|Follow-up ** Monitoring|Monitoring ** other surveys|Other surveys * Tools ** links|Links ** people|People ** currentevents-url|currentevents ** recentchanges-url|recentchanges ** randompage-url|randompage ** helppage|help * SEARCH * TOOLBOX 7283a1cd32e16ff1d0178ff4fe8d8a6547c1a33f 0 359 2818 2023-05-15T13:32:05Z Gsawgwikiadmin 1 Created page with "== Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held Workshop2023:logis..." wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valetta at the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. d36364f318bc21a371170db155b2cf60676e0861 2828 2818 2023-05-17T12:18:10Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta at the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Maja Jablonska (Warsaw) * Marius Maskoliunas (Vilnius) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. 4bdbf527368cde8394a075c44c6896a641ab33e9 2830 2828 2023-05-30T10:15:51Z Gsawgwikiadmin 1 /* Workshop Organising Committee */ wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta at the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. bd4d98c2c2c79dc429e9b3ece3f3b328ca5374b8 2831 2830 2023-05-30T12:38:52Z Gsawgwikiadmin 1 /* Welcome! */ wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. 6e30539059b9716313a3ccbf11349cef93b554e2 2834 2831 2023-06-24T07:35:01Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[Media:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. 2ca998f691665e1f59bb88a8822f370f30454f2e 2835 2834 2023-06-24T07:35:20Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. 6e30539059b9716313a3ccbf11349cef93b554e2 2837 2835 2023-06-24T07:36:07Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[File:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. fe388c11fde7b845421f2e7e999eda6777c8b09b 2839 2837 2023-06-24T07:36:29Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported jointly by the EC H2020 ORP grant no 101004719. 6e30539059b9716313a3ccbf11349cef93b554e2 2857 2839 2023-10-02T18:12:29Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] [[File:Malta2023.png|right|350px|Photo]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported by the EC H2020 ORP grant no 101004719. 71b07a51bafd46d84ab266bbce7a01c2197c551b 0 360 2819 2023-05-15T15:18:00Z Gsawgwikiadmin 1 Created page with "Preliminary agenda ---- '''Mon 2.10''' 12:30 lunch 14:00 start of the workshop 18:00 end of day 1 '''Tue 3.10''' 09:00 start of day 2 18:00 end of day 2 '''Wed 4.10'''..." wikitext text/x-wiki Preliminary agenda ---- '''Mon 2.10''' 12:30 lunch 14:00 start of the workshop 18:00 end of day 1 '''Tue 3.10''' 09:00 start of day 2 18:00 end of day 2 '''Wed 4.10''' 09:00 start of day 3 18:00 end of day 3 '''Thu 5.10''' 09:00 start of day 4 16:15 end of day 4 TBC: conference dinner '''Fri 6.10''' informal discussion/trip f70d57bddb92715986ed6751a01953ebe569b870 2847 2819 2023-09-19T21:51:19Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- Preliminary agenda ---- '''Mon 2.10''' 12:30 lunch 14:00 start of the workshop 18:00 end of day 1 '''Tue 3.10''' 09:00 start of day 2 18:00 end of day 2 '''Wed 4.10''' 09:00 start of day 3 18:00 end of day 3 '''Thu 5.10''' 09:00 start of day 4 16:15 end of day 4 TBC: conference dinner '''Fri 6.10''' informal discussion/trip 0c40ef74ce7999106715ae75bc44266bd1b4448c 2849 2847 2023-09-22T19:16:41Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing] ---- '''Mon 2.10''' 12:30 lunch 14:00 start of the workshop 18:00 end of day 1 '''Tue 3.10''' 09:30 start of day 2 18:00 end of day 2 '''Wed 4.10''' 09:30 start of day 3 18:00 end of day 3 '''Thu 5.10''' 09:30 start of day 4 16:15 end of day 4 TBC: conference dinner '''Fri 6.10''' focus groups/trip 7e929ba7b5fa7fa23d86ca79c8fde80082b93077 2850 2849 2023-09-22T19:16:54Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] ---- '''Mon 2.10''' 12:30 lunch 14:00 start of the workshop 18:00 end of day 1 '''Tue 3.10''' 09:30 start of day 2 18:00 end of day 2 '''Wed 4.10''' 09:30 start of day 3 18:00 end of day 3 '''Thu 5.10''' 09:30 start of day 4 16:15 end of day 4 TBC: conference dinner '''Fri 6.10''' focus groups/trip 92409253da710da7257a07150dd2619f8d78a8af 2851 2850 2023-09-24T08:08:58Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. 103a09ed6f2abe11f1b68af957b78fdb5bd22134 2852 2851 2023-09-24T08:09:11Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- <big>Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] </big> ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. f97ff9475d6917be047bd56c8b5dcf838b33a716 2853 2852 2023-09-24T08:09:19Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- <big>'''Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] '''</big> ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. d22a59398488220966505c19f2bc2979676b07e7 2856 2853 2023-10-01T07:07:39Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- <big>'''Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] '''</big> ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. ---- YouTube streams and recordings: * [https://youtube.com/live/0caDKj6brCk?feature=share Monday from 2pm CEST] d6f92d5193578d8aa859ddf10babc6b307e64ea7 0 361 2820 2023-05-15T15:18:33Z Gsawgwikiadmin 1 Created page with "Registration will open soon and will close on Sep.10,2023." wikitext text/x-wiki Registration will open soon and will close on Sep.10,2023. 6aa61776cd1ece0835e57291f031a42d4f0d27d9 2829 2820 2023-05-17T12:44:37Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is OPEN until 1.September 2022]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' 185c730ce970254ac589d6c340f997457fe5884d 2840 2829 2023-08-30T13:11:08Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is OPEN until 1.September 2023]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' fd736f8f1cfabfda1af708f5c24f1fe5fc71b784 2841 2840 2023-09-19T21:25:38Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is OPEN until 1.September 2023]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- Registered participants #Dr. Agnieszka Słowikowska JIVE/NCU #Dr. Alex Markowitz Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences #Dr. Alexios Liakos IAASARS, National Observatory of Athens #Dr. Andrii Simon Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv #Dr. Areg Mickaelian Byurakan Astrophysical Observatory (BAO) #Mr Ashwin Varma Nicolaus Copernicus University #Mrs Barbara Handzlik Astronomical Observatory of the Jagiellonian University #Mrs Bartosz Kirpluk The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń #Dr. Basa Stéphane LAM #Dr. Ben Dryer The Open University #Prof. Charles Galdies University of Malta #Dr. Dawid Moździerski University of Wrocław #Dr. Edyta Podlewska-Gaca Astronomical Observatory Institute, Adam Mickiewicz University #Dr. Enrique Solano Centro de Astrobiología (INTA-CSIC) #Dr. Fabian Schussler IRFU / CEA Paris-Saclay #Dr. Felice Cusano INAF OAS-Bologna #Dr. Franz-Josef Hambsch ROAD Observatory #Dr. Fraser Lewis Faulkes Telescope Project #Dr. Gamal Hamed National Research Institute of Astronomy and Geophysics #Prof. Gerry Gilmore IoA Cambridge #Dr. Gudrun Tausch-Pebody IoA Cambridge #Dr. Ilse van Bemmel JIVE #Dr. Jaroslav Merc Astronomical Institute of Charles University #Dr. Joanna Molenda-Zakowicz University of Wroclaw, Department of Physics and Astronomy #Mrs Justyna Olszewska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University in Poznań #Dr. Karolina Bąkowska N. Copernicus University in Torun #Dr. Katarzyna Kruszynska Astronomical Observatory, University of Warsaw #Mrs Kaziemova Kristina Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv. #Mr Kornel Howil Astronomical Observatory, University of Warsaw #Prof. Lukasz Wyrzykowski Warsaw University Astronomical Observatory #Dr. Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University #Mr Michal Zejmo Janusz Gil Institute of Astronomy, University of Zielona Gora #Mrs Nada Ihanec Astronomical Observatory University of Warsaw #Mrs. Oleksandra Pyshna Astronomical Observatory of Taras Shevchenko National University of Kyiv #Dr. Paolo Rota Università degli Studi di Salerno #Mr Patrik Sivak Astronomical Observatory of the University of Warsaw #Dr. Paweł Zieliński The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń #Mr Piotr Trzcionkowski Obserwatorium Astronomiczne UW #Mr Przemyslaw J. Mikolajczyk Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wroclaw #Dr. Rachel Street Las Cumbres Observatory #Dr. Rupak Roy Manipal Academy of Higher Education (MAHE) #Mr Sebastian Kurowski Astronomical Observatory of the Jagiellonian University #Dr. Siegfried Vanaverbeke Vereniging voor sterrenkunde #Dr. Simon Hodgkin Institute of Astronomy, Cambridge University #Prof. Staszek Zola Jagiellonian University #Mr Stefan Stefanov Institute of Astronomy & Rozhen Observatory, Bulgarian Academy of Sciences #Mr Stephen Brincat AAVSO #Prof. Stephen Potter South African Astronomical Observatory #Dr. Steve Fossey UCL #Mr Tathagata Saha Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw #Dr. Thomas Wevers STScI #Dr. Tom Esposito SETI Institute / Unistellar #Mrs Uliana Pylypenko Astronomical Observatory of the University of Warsaw #Prof. Wyn Evans University of Cambridge #Dr. Yanko Nikolov Institute of Astronomy and National Astronomical Observatory #Dr. Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences a1dc591ee7e060790d3550f5d854725d5360141e 2842 2841 2023-09-19T21:46:24Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is OPEN until 1.September 2023]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' We can only accommodate 50 attendees on-site. The submitted registrations will be reviewed by the Workshop Organizing Committee and the accepted attendees will be selected. The streaming will be available openly. '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- Registered participants #Dr. Agnieszka Słowikowska JIVE/NCU #Dr. Alex Markowitz Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences #Dr. Alexios Liakos IAASARS, National Observatory of Athens #Dr. Andrii Simon Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv #Dr. Areg Mickaelian Byurakan Astrophysical Observatory (BAO) #Mr Ashwin Varma Nicolaus Copernicus University #Mrs Barbara Handzlik Astronomical Observatory of the Jagiellonian University #Mrs Bartosz Kirpluk The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. #Dr. Basa Stéphane LAM #Dr. Ben Dryer The Open University #Prof. Charles Galdies University of Malta #Dr. Dawid Moździerski University of Wrocław #Dr. Edyta Podlewska-Gaca Astronomical Observatory Institute, Adam Mickiewicz University #Dr. Enrique Solano Centro de Astrobiología (INTA-CSIC) #Dr. Fabian Schussler IRFU / CEA Paris-Saclay #Dr. Felice Cusano INAF OAS-Bologna #Dr. Franz-Josef Hambsch ROAD Observatory #Dr. Fraser Lewis Faulkes Telescope Project #Dr. Gamal Hamed National Research Institute of Astronomy and Geophysics #Prof. Gerry Gilmore IoA Cambridge #Dr. Gudrun Tausch-Pebody IoA Cambridge #Dr. Ilse van Bemmel JIVE #Dr. Jaroslav Merc Astronomical Institute of Charles University #Dr. Joanna Molenda-Zakowicz University of Wroclaw, Department of Physics and Astronomy #Mrs Justyna Olszewska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University in Poznań #Dr. Karolina Bąkowska N. Copernicus University in Torun #Dr. Katarzyna Kruszynska Astronomical Observatory, University of Warsaw #Mrs Kaziemova Kristina Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv. #Mr Kornel Howil Astronomical Observatory, University of Warsaw #Prof. Lukasz Wyrzykowski Warsaw University Astronomical Observatory #Dr. Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University #Dr. Mariusz Gromadzki Astronomical Observatory, University of Warsaw #Mr Michal Zejmo Janusz Gil Institute of Astronomy, University of Zielona Gora #Prof. Michel Dennefeld IAP/Paris, CNRS & Sorbonne University #Dr. Milena Ratajczak University of Warsaw #Mrs. Monika Sitek Astronomical Observatory, University of Warsaw #Mrs Nada Ihanec Astronomical Observatory University of Warsaw #Mrs. Oleksandra Pyshna Astronomical Observatory of Taras Shevchenko National University of Kyiv #Dr. Paolo Rota Università degli Studi di Salerno #Mr Patrik Sivak Astronomical Observatory of the University of Warsaw #Dr. Paweł Zieliński Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland #Mr Piotr Trzcionkowski Astronomical Observatory, University of Warsaw #Mr Przemyslaw J. Mikolajczyk Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wroclaw #Dr. Rachel Street Las Cumbres Observatory #Dr. Rupak Roy Manipal Academy of Higher Education (MAHE) #Mr Sebastian Kurowski Astronomical Observatory of the Jagiellonian University #Dr. Siegfried Vanaverbeke Vereniging voor sterrenkunde #Dr. Simon Hodgkin Institute of Astronomy, Cambridge University #Prof. Staszek Zola Jagiellonian University #Mr Stefan Stefanov Institute of Astronomy & Rozhen Observatory, Bulgarian Academy of Sciences #Mr Stephen Brincat AAVSO #Prof. Stephen Potter South African Astronomical Observatory #Dr. Steve Fossey UCL #Mr Tathagata Saha Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw #Dr. Thomas Wevers STScI #Dr. Tom Esposito SETI Institute / Unistellar #Mrs Uliana Pylypenko Astronomical Observatory of the University of Warsaw #Prof. Wyn Evans University of Cambridge #Dr. Yanko Nikolov Institute of Astronomy and National Astronomical Observatory #Dr. Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 4b02dde0f41c60cd7c1f1beb828047dd907e2b7c 2843 2842 2023-09-19T21:46:50Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is OPEN until 1.September 2023]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- Registered participants #Dr. Agnieszka Słowikowska JIVE/NCU #Dr. Alex Markowitz Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences #Dr. Alexios Liakos IAASARS, National Observatory of Athens #Dr. Andrii Simon Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv #Dr. Areg Mickaelian Byurakan Astrophysical Observatory (BAO) #Mr Ashwin Varma Nicolaus Copernicus University #Mrs Barbara Handzlik Astronomical Observatory of the Jagiellonian University #Mrs Bartosz Kirpluk The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. #Dr. Basa Stéphane LAM #Dr. Ben Dryer The Open University #Prof. Charles Galdies University of Malta #Dr. Dawid Moździerski University of Wrocław #Dr. Edyta Podlewska-Gaca Astronomical Observatory Institute, Adam Mickiewicz University #Dr. Enrique Solano Centro de Astrobiología (INTA-CSIC) #Dr. Fabian Schussler IRFU / CEA Paris-Saclay #Dr. Felice Cusano INAF OAS-Bologna #Dr. Franz-Josef Hambsch ROAD Observatory #Dr. Fraser Lewis Faulkes Telescope Project #Dr. Gamal Hamed National Research Institute of Astronomy and Geophysics #Prof. Gerry Gilmore IoA Cambridge #Dr. Gudrun Tausch-Pebody IoA Cambridge #Dr. Ilse van Bemmel JIVE #Dr. Jaroslav Merc Astronomical Institute of Charles University #Dr. Joanna Molenda-Zakowicz University of Wroclaw, Department of Physics and Astronomy #Mrs Justyna Olszewska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University in Poznań #Dr. Karolina Bąkowska N. Copernicus University in Torun #Dr. Katarzyna Kruszynska Astronomical Observatory, University of Warsaw #Mrs Kaziemova Kristina Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv. #Mr Kornel Howil Astronomical Observatory, University of Warsaw #Prof. Lukasz Wyrzykowski Warsaw University Astronomical Observatory #Dr. Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University #Dr. Mariusz Gromadzki Astronomical Observatory, University of Warsaw #Mr Michal Zejmo Janusz Gil Institute of Astronomy, University of Zielona Gora #Prof. Michel Dennefeld IAP/Paris, CNRS & Sorbonne University #Dr. Milena Ratajczak University of Warsaw #Mrs. Monika Sitek Astronomical Observatory, University of Warsaw #Mrs Nada Ihanec Astronomical Observatory University of Warsaw #Mrs. Oleksandra Pyshna Astronomical Observatory of Taras Shevchenko National University of Kyiv #Dr. Paolo Rota Università degli Studi di Salerno #Mr Patrik Sivak Astronomical Observatory of the University of Warsaw #Dr. Paweł Zieliński Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland #Mr Piotr Trzcionkowski Astronomical Observatory, University of Warsaw #Mr Przemyslaw J. Mikolajczyk Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wroclaw #Dr. Rachel Street Las Cumbres Observatory #Dr. Rupak Roy Manipal Academy of Higher Education (MAHE) #Mr Sebastian Kurowski Astronomical Observatory of the Jagiellonian University #Dr. Siegfried Vanaverbeke Vereniging voor sterrenkunde #Dr. Simon Hodgkin Institute of Astronomy, Cambridge University #Prof. Staszek Zola Jagiellonian University #Mr Stefan Stefanov Institute of Astronomy & Rozhen Observatory, Bulgarian Academy of Sciences #Mr Stephen Brincat AAVSO #Prof. Stephen Potter South African Astronomical Observatory #Dr. Steve Fossey UCL #Mr Tathagata Saha Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw #Dr. Thomas Wevers STScI #Dr. Tom Esposito SETI Institute / Unistellar #Mrs Uliana Pylypenko Astronomical Observatory of the University of Warsaw #Prof. Wyn Evans University of Cambridge #Dr. Yanko Nikolov Institute of Astronomy and National Astronomical Observatory #Dr. Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 9efa5862afb79951b5ca0875d16c3c6c10d8a530 2848 2843 2023-09-21T13:48:53Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is CLOSED]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- Registered participants #Dr. Agnieszka Słowikowska JIVE/NCU #Dr. Alex Markowitz Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences #Dr. Alexios Liakos IAASARS, National Observatory of Athens #Dr. Andrii Simon Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv #Dr. Areg Mickaelian Byurakan Astrophysical Observatory (BAO) #Mr Ashwin Varma Nicolaus Copernicus University #Mrs Barbara Handzlik Astronomical Observatory of the Jagiellonian University #Mrs Bartosz Kirpluk The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. #Dr. Basa Stéphane LAM #Dr. Ben Dryer The Open University #Prof. Charles Galdies University of Malta #Dr. Dawid Moździerski University of Wrocław #Dr. Edyta Podlewska-Gaca Astronomical Observatory Institute, Adam Mickiewicz University #Dr. Enrique Solano Centro de Astrobiología (INTA-CSIC) #Dr. Fabian Schussler IRFU / CEA Paris-Saclay #Dr. Felice Cusano INAF OAS-Bologna #Dr. Franz-Josef Hambsch ROAD Observatory #Dr. Fraser Lewis Faulkes Telescope Project #Dr. Gamal Hamed National Research Institute of Astronomy and Geophysics #Prof. Gerry Gilmore IoA Cambridge #Dr. Gudrun Tausch-Pebody IoA Cambridge #Dr. Ilse van Bemmel JIVE #Dr. Jaroslav Merc Astronomical Institute of Charles University #Dr. Joanna Molenda-Zakowicz University of Wroclaw, Department of Physics and Astronomy #Mrs Justyna Olszewska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University in Poznań #Dr. Karolina Bąkowska N. Copernicus University in Torun #Dr. Katarzyna Kruszynska Astronomical Observatory, University of Warsaw #Mrs Kaziemova Kristina Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv. #Mr Kornel Howil Astronomical Observatory, University of Warsaw #Prof. Lukasz Wyrzykowski Warsaw University Astronomical Observatory #Dr. Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University #Dr. Mariusz Gromadzki Astronomical Observatory, University of Warsaw #Mr Michal Zejmo Janusz Gil Institute of Astronomy, University of Zielona Gora #Prof. Michel Dennefeld IAP/Paris, CNRS & Sorbonne University #Dr. Milena Ratajczak University of Warsaw #Mrs. Monika Sitek Astronomical Observatory, University of Warsaw #Mrs Nada Ihanec Astronomical Observatory University of Warsaw #Mrs. Oleksandra Pyshna Astronomical Observatory of Taras Shevchenko National University of Kyiv #Dr. Paolo Rota Università degli Studi di Salerno #Mr Patrik Sivak Astronomical Observatory of the University of Warsaw #Dr. Paweł Zieliński Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland #Mr Piotr Trzcionkowski Astronomical Observatory, University of Warsaw #Mr Przemyslaw J. Mikolajczyk Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wroclaw #Dr. Rachel Street Las Cumbres Observatory #Dr. Rupak Roy Manipal Academy of Higher Education (MAHE) #Mr Sebastian Kurowski Astronomical Observatory of the Jagiellonian University #Dr. Siegfried Vanaverbeke Vereniging voor sterrenkunde #Dr. Simon Hodgkin Institute of Astronomy, Cambridge University #Prof. Staszek Zola Jagiellonian University #Mr Stefan Stefanov Institute of Astronomy & Rozhen Observatory, Bulgarian Academy of Sciences #Mr Stephen Brincat AAVSO #Prof. Stephen Potter South African Astronomical Observatory #Dr. Steve Fossey UCL #Mr Tathagata Saha Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw #Dr. Thomas Wevers STScI #Dr. Tom Esposito SETI Institute / Unistellar #Mrs Uliana Pylypenko Astronomical Observatory of the University of Warsaw #Prof. Wyn Evans University of Cambridge #Dr. Yanko Nikolov Institute of Astronomy and National Astronomical Observatory #Dr. Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 7cd5d697315f59cddb283926d5bf12b0d2ea4d69 2854 2848 2023-09-24T13:41:42Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is CLOSED]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- Registered participants #Dr. Agnieszka Słowikowska JIVE/NCU #Dr. Alex Markowitz Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences #Dr. Alexios Liakos IAASARS, National Observatory of Athens #Dr. Andrii Simon Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv #Dr. Areg Mickaelian Byurakan Astrophysical Observatory (BAO) #Mr Ashwin Varma Nicolaus Copernicus University #Mrs Barbara Handzlik Astronomical Observatory of the Jagiellonian University #Mrs Bartosz Kirpluk The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. #Dr. Basa Stéphane LAM #Dr. Ben Dryer The Open University #Prof. Charles Galdies University of Malta #Dr. Cosimo Insera University of Cardiff #Dr. Dawid Moździerski University of Wrocław #Dr. Edyta Podlewska-Gaca Astronomical Observatory Institute, Adam Mickiewicz University #Dr. Enrique Solano Centro de Astrobiología (INTA-CSIC) #Dr. Fabian Schussler IRFU / CEA Paris-Saclay #Dr. Felice Cusano INAF OAS-Bologna #Dr. Franz-Josef Hambsch ROAD Observatory #Dr. Fraser Lewis Faulkes Telescope Project #Dr. Gamal Hamed National Research Institute of Astronomy and Geophysics #Prof. Gerry Gilmore IoA Cambridge #Dr. Gudrun Tausch-Pebody IoA Cambridge #Dr. Ilse van Bemmel JIVE #Dr. Jaroslav Merc Astronomical Institute of Charles University #Dr. Joanna Molenda-Zakowicz University of Wroclaw, Department of Physics and Astronomy #Mrs Justyna Olszewska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University in Poznań #Dr. Karolina Bąkowska N. Copernicus University in Torun #Dr. Katarzyna Kruszynska Astronomical Observatory, University of Warsaw #Mrs Kaziemova Kristina Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv. #Mr Kornel Howil Astronomical Observatory, University of Warsaw #Prof. Lukasz Wyrzykowski Warsaw University Astronomical Observatory #Dr. Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University #Dr. Mariusz Gromadzki Astronomical Observatory, University of Warsaw #Mr Michal Zejmo Janusz Gil Institute of Astronomy, University of Zielona Gora #Prof. Michel Dennefeld IAP/Paris, CNRS & Sorbonne University #Dr. Milena Ratajczak University of Warsaw #Mrs. Monika Sitek Astronomical Observatory, University of Warsaw #Mrs Nada Ihanec Astronomical Observatory University of Warsaw #Mrs. Oleksandra Pyshna Astronomical Observatory of Taras Shevchenko National University of Kyiv #Dr. Paolo Rota Università degli Studi di Salerno #Mr Patrik Sivak Astronomical Observatory of the University of Warsaw #Dr. Paweł Zieliński Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland #Mr Piotr Trzcionkowski Astronomical Observatory, University of Warsaw #Mr Przemyslaw J. Mikolajczyk Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wroclaw #Dr. Rachel Street Las Cumbres Observatory #Dr. Rupak Roy Manipal Academy of Higher Education (MAHE) #Mr Sebastian Kurowski Astronomical Observatory of the Jagiellonian University #Dr. Siegfried Vanaverbeke Vereniging voor sterrenkunde #Dr. Simon Hodgkin Institute of Astronomy, Cambridge University #Prof. Staszek Zola Jagiellonian University #Mr Stefan Stefanov Institute of Astronomy & Rozhen Observatory, Bulgarian Academy of Sciences #Mr Stephen Brincat AAVSO #Prof. Stephen Potter South African Astronomical Observatory #Dr. Steve Fossey UCL #Mr Tathagata Saha Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw #Dr. Thomas Wevers STScI #Dr. Tom Esposito SETI Institute / Unistellar #Mrs Uliana Pylypenko Astronomical Observatory of the University of Warsaw #Prof. Wyn Evans University of Cambridge #Dr. Yanko Nikolov Institute of Astronomy and National Astronomical Observatory #Dr. Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences 46811c2ea57d12a80c257307c234e8b18c8011d5 2855 2854 2023-09-25T09:24:15Z Gsawgwikiadmin 1 wikitext text/x-wiki <big>'''[https://forms.gle/YvqFeEXy8JyrotCj9 Registration is CLOSED]'''</big> '''The workshop will be held both physically and in the online space (streaming and allowing for remote participation).''' '''There is no registration fee - as always at our workshops! This year we thank the ORP H2020 grant again. ''' ---- Registered participants #Dr. Agnieszka Słowikowska JIVE/NCU #Dr. Alex Markowitz Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences #Dr. Alexios Liakos IAASARS, National Observatory of Athens #Prof. Andreja Gomboc University of Nova Gorica #Dr. Andrii Simon Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv #Dr. Areg Mickaelian Byurakan Astrophysical Observatory (BAO) #Mr Ashwin Varma Nicolaus Copernicus University #Mrs Barbara Handzlik Astronomical Observatory of the Jagiellonian University #Mrs Bartosz Kirpluk The Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Toruń, Poland. #Dr. Basa Stéphane LAM #Dr. Ben Dryer The Open University #Prof. Charles Galdies University of Malta #Dr. Cosimo Insera University of Cardiff #Dr. Dawid Moździerski University of Wrocław #Dr. Edyta Podlewska-Gaca Astronomical Observatory Institute, Adam Mickiewicz University #Mr. Eldho Sunny Mar Athanasius College, Kothamangalam #Dr. Enrique Solano Centro de Astrobiología (INTA-CSIC) #Dr. Fabian Schussler IRFU / CEA Paris-Saclay #Dr. Felice Cusano INAF OAS-Bologna #Dr. Franz-Josef Hambsch ROAD Observatory #Dr. Fraser Lewis Faulkes Telescope Project #Dr. Gamal Hamed National Research Institute of Astronomy and Geophysics #Prof. Gerry Gilmore IoA Cambridge #Dr. Gudrun Tausch-Pebody IoA Cambridge #Dr. Ilse van Bemmel JIVE #Dr. Jaroslav Merc Astronomical Institute of Charles University #Dr. Joanna Molenda-Zakowicz University of Wroclaw, Department of Physics and Astronomy #Mrs Justyna Olszewska Astronomical Observatory Institute, Faculty of Physics, Adam Mickiewicz University in Poznań #Dr. Karolina Bąkowska N. Copernicus University in Torun #Dr. Katarzyna Kruszynska Astronomical Observatory, University of Warsaw #Mrs Kaziemova Kristina Astronomy and Space Physics Department, Taras Shevchenko National University of Kyiv. #Mr Kornel Howil Astronomical Observatory, University of Warsaw #Dr. Laurent Eyer Geneva Observatory #Prof. Lukasz Wyrzykowski Warsaw University Astronomical Observatory #Mr. Mateusz Bronikowski University of Nova Gorica #Dr. Marius Maskoliunas Institute of Theoretical Physics and Astronomy, Vilnius University #Dr. Mariusz Gromadzki Astronomical Observatory, University of Warsaw #Mr Michal Zejmo Janusz Gil Institute of Astronomy, University of Zielona Gora #Prof. Michel Dennefeld IAP/Paris, CNRS & Sorbonne University #Dr. Milena Ratajczak University of Warsaw #Mrs. Monika Sitek Astronomical Observatory, University of Warsaw #Mrs Nada Ihanec Astronomical Observatory University of Warsaw #Mrs. Oleksandra Pyshna Astronomical Observatory of Taras Shevchenko National University of Kyiv #Dr. Paolo Rota Università degli Studi di Salerno #Mr Patrik Sivak Astronomical Observatory of the University of Warsaw #Dr. Paweł Zieliński Institute of Astronomy, Nicolaus Copernicus University in Toruń, Poland #Mr Piotr Trzcionkowski Astronomical Observatory, University of Warsaw #Mr Przemyslaw J. Mikolajczyk Astronomical Observatory, University of Warsaw; Astronomical Institute, University of Wroclaw #Dr. Rachel Street Las Cumbres Observatory #Dr. Rupak Roy Manipal Academy of Higher Education (MAHE) #Mr Sebastian Kurowski Astronomical Observatory of the Jagiellonian University #Dr. Siegfried Vanaverbeke Vereniging voor sterrenkunde #Dr. Simon Hodgkin Institute of Astronomy, Cambridge University #Prof. Staszek Zola Jagiellonian University #Mr Stefan Stefanov Institute of Astronomy & Rozhen Observatory, Bulgarian Academy of Sciences #Mr Stephen Brincat AAVSO #Prof. Stephen Potter South African Astronomical Observatory #Dr. Steve Fossey UCL #Mr Tathagata Saha Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, Warsaw #Dr. Thomas Wevers STScI #Dr. Tom Esposito SETI Institute / Unistellar #Mrs Uliana Pylypenko Astronomical Observatory of the University of Warsaw #Prof. Wyn Evans University of Cambridge #Dr. Yanko Nikolov Institute of Astronomy and National Astronomical Observatory #Dr. Zsofia Nagy Konkoly Observatory, Research Centre for Astronomy and Earth Sciences a6e3d924063392712e689bfa5a73d84ed14eae97 0 362 2821 2023-05-17T12:14:45Z Gsawgwikiadmin 1 Created page with "= Venue = [Embassy Hotel, Valletta https://www.embassyvallettahotel.com/]" wikitext text/x-wiki = Venue = [Embassy Hotel, Valletta https://www.embassyvallettahotel.com/] 09a404e4ceb06c23f16c3f49085a6ad111533521 2822 2821 2023-05-17T12:14:56Z Gsawgwikiadmin 1 wikitext text/x-wiki = Venue = [[Embassy Hotel, Valletta https://www.embassyvallettahotel.com/]] 534ead5c5db3bc0c9ca0dee05190d120f3b20b59 2823 2822 2023-05-17T12:15:08Z Gsawgwikiadmin 1 wikitext text/x-wiki = Venue = Embassy Hotel, Valletta [[https://www.embassyvallettahotel.com/]] 018a474b52efb86218c17352c8ab012d294e5011 2824 2823 2023-05-17T12:15:18Z Gsawgwikiadmin 1 wikitext text/x-wiki = Venue = Embassy Hotel, Valletta [https://www.embassyvallettahotel.com/] cf44799728887566f773ebfe9b4b6ade20665e5e 2825 2824 2023-05-17T12:15:29Z Gsawgwikiadmin 1 wikitext text/x-wiki = Venue = [https://www.embassyvallettahotel.com/ | Embassy Hotel, Valletta] 6fdec53763c5f3daa660b3a1ad4b8c5865b64c0a 2826 2825 2023-05-17T12:15:38Z Gsawgwikiadmin 1 wikitext text/x-wiki = Venue = [https://www.embassyvallettahotel.com/ Embassy Hotel, Valletta] e24c79cae587d7cfbaa31ba892408471375323c9 2827 2826 2023-05-17T12:17:54Z Gsawgwikiadmin 1 wikitext text/x-wiki = Venue = [https://www.embassyvallettahotel.com/ Embassy Hotel] in the Valletta city centre. = Airport = [https://www.maltairport.com/ Malta International Airport] 30f85d09c16f9ef427854e113b0907c6b5e7c36f 6 363 2832 2023-05-30T12:40:04Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2836 2832 2023-06-24T07:35:39Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2023-small.png]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 6 364 2833 2023-05-30T13:11:00Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 2838 2833 2023-06-24T07:36:20Z Gsawgwikiadmin 1 Gsawgwikiadmin uploaded a new version of [[File:Poster2023.pdf]] wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 365 2844 2023-09-19T21:47:54Z Gsawgwikiadmin 1 Created page with "* Gaia Alerts" wikitext text/x-wiki * Gaia Alerts 73d18c15863dbb3982df93e5b364bff006a76045 2845 2844 2023-09-19T21:49:00Z Gsawgwikiadmin 1 wikitext text/x-wiki * Gaia mission and Alerts * BHTOM follow-up system * highlights and results * synergies with radio, X, GW * telescope network * organization * opportunities 3c746ed7478be125d4384e951f7889a769184280 2846 2845 2023-09-19T21:49:48Z Gsawgwikiadmin 1 wikitext text/x-wiki * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes 19e1a3d7015b59ef123e7de8711274f9e3b4fc18 0 360 2858 2856 2023-10-02T18:34:44Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- <big>'''Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] '''</big> ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. ---- YouTube streams and recordings: * [https://youtube.com/live/0caDKj6brCk?feature=share Monday from 2pm CEST] * [https://youtube.com/live/jzlkFjEZVz0?feature=share Tuesday from 9:30 CEST] 1f8fa7ceaa8bba0c02824b024e0376f2ec26daf2 2863 2858 2023-10-03T15:05:05Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- <big>'''Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] '''</big> ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. ---- YouTube streams and recordings: * [https://youtube.com/live/0caDKj6brCk?feature=share Monday from 2pm CEST] * [https://youtube.com/live/jzlkFjEZVz0?feature=share Tuesday from 9:30 CEST] * [https://youtube.com/live/8thpT4Ebb1g?feature=share Wednesday from 9:30 CEST] c648fa7e01434872f06fef1380587e1a024a0873 2864 2863 2023-10-05T07:35:17Z Gsawgwikiadmin 1 wikitext text/x-wiki '''The workshop will be streamed via YouTube on the Warsaw University Astronomical Observatory channel''' ---- <big>'''Draft agenda [https://docs.google.com/spreadsheets/d/1nvB-rFD1Aesyg9L126EPPIfJEHCbUgvObYXkUJTNUSc/edit?usp=sharing HERE] '''</big> ---- We start the workshop on Mon 2.10 with lunch at 12:30 and first talk at 14:00 CEST. Conference dinner on Thu. Friday will be dedicated to focus group meetings and/or a trip. ---- YouTube streams and recordings: * [https://youtube.com/live/0caDKj6brCk?feature=share Monday from 2pm CEST] * [https://youtube.com/live/jzlkFjEZVz0?feature=share Tuesday from 9:30 CEST] * [https://youtube.com/live/8thpT4Ebb1g?feature=share Wednesday from 9:30 CEST] * [https://youtube.com/live/TaxvIQx4cLM?feature=share Thursday from 9:30 CEST] d8cc98d7d42911aebb3c6fdb676f3bef22a4ff49 6 366 2859 2023-10-02T18:40:44Z Gsawgwikiadmin 1 wikitext text/x-wiki da39a3ee5e6b4b0d3255bfef95601890afd80709 0 359 2860 2857 2023-10-02T18:41:08Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] [[File:Malta2023.jpg|right|350px|Photo]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported by the EC H2020 ORP grant no 101004719. 5b06c868cb8fa73b7c14522458100892e3dccad9 2861 2860 2023-10-02T18:41:32Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] [[File:Malta2023.jpg|right|550px|Photo]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported by the EC H2020 ORP grant no 101004719. 770003b29e480c300654a453f5815abb4f860bac 2862 2861 2023-10-02T18:41:45Z Gsawgwikiadmin 1 wikitext text/x-wiki == Welcome! == [[File:Poster2023-small.png|right|350px|poster2023]] '''The 14th Gaia Science Alerts workshop and the ORP Time-Domain meeting will be held [[Workshop2023:logistics | in Valletta on the island of Malta, and online 2-5 October 2023]]''' The main goals of the workshop are: * update on the Gaia mission * update on the Gaia Alerts * update on the BHTOM follow-up system * Gaia Alerts highlights and results in transient astronomy (supernovae, microlensing, novae) * synergies with radio within the new OPTICON-RadioNET Pilot (ORP) grant * new members of the telescope network * organization of the follow-up * opportunities for small and mid-sized telescopes ---- * [[workshop2023:rationale|Rationale]] * [[workshop2023:agenda|Agenda]] * [[workshop2023:registration|Registration]] * [[workshop2023:logistics|Logistical information]] * [[Media:Poster2023.pdf|Poster for download]] [[File:Malta2023.jpg|right|750px|Photo]] ---- === Workshop Organising Committee === Workshop Organising Committee: * Lukasz Wyrzykowski (Warsaw) * Milena Ratajczak (Warsaw) * Simon Hodgkin (Cambridge) * Charles Galdies (Malta) * Stephen M. Brincat (Malta) * Gerry Gilmore (Cambridge) * Nada Ihanec (Warsaw) The workshop is supported by the EC H2020 ORP grant no 101004719. 64ecc2b18cf2547a53b6992adb5400917e9c7349